Question coercivity hdds

nandobadam88

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HFF 2.5" models WD10JPVX-08JC3T5, HGST HTS541010A99E662, ST500LM030 is low or high coercivity?
 

Solution
Short answer — they use high‑coercivity thin‑film media (i.e., modern HDD platter materials), not the low‑coercivity media you see in old floppy/tape. The three models you named differ in recording method, but all are built from modern, high‑coercivity platter materials designed to resist stray magnetic fields.
Details:
  • Seagate ST500LM030 — Seagate Barracuda mobile 2.5" — uses SMR (shingled magnetic recording). SMR is a track‑layout choice, but the underlying platters are still modern thin‑film media with high coercivity.
  • WDC WD10JPVX‑08JC3T5 — Western Digital Blue 2.5" — uses CMR (conventional/PMR style), also on modern high‑coercivity platters.
  • HGST HTS541010A99E662 (Travelstar) — CMR (PMR family), again modern thin‑film...
Short answer — they use high‑coercivity thin‑film media (i.e., modern HDD platter materials), not the low‑coercivity media you see in old floppy/tape. The three models you named differ in recording method, but all are built from modern, high‑coercivity platter materials designed to resist stray magnetic fields.
Details:
  • Seagate ST500LM030 — Seagate Barracuda mobile 2.5" — uses SMR (shingled magnetic recording). SMR is a track‑layout choice, but the underlying platters are still modern thin‑film media with high coercivity.
  • WDC WD10JPVX‑08JC3T5 — Western Digital Blue 2.5" — uses CMR (conventional/PMR style), also on modern high‑coercivity platters.
  • HGST HTS541010A99E662 (Travelstar) — CMR (PMR family), again modern thin‑film high‑coercivity media.
Important caveat:
  • Manufacturers generally do not publish raw coercivity numbers (kA/m or Oe) for consumer drives, so you will not find an official “coercivity = X” in typical datasheets. The practical takeaway is that these laptop drives use media engineered with much higher coercivity than old magnetic media, so they’re far more resistant to ordinary household magnets and CRT stray fields.
Practical implication:
  • “High coercivity” means a nearby switched‑off CRT or small speaker magnets at a few centimetres is very unlikely to demagnetize or corrupt data on these drives. Only very strong fields (industrial degaussers or extremely large/close permanent magnets) or direct physical damage/sensor faults are realistic threats. Still, simple precautions — move drives a few tens of centimetres away and keep backups — are sensible.
If you want:
  • I can give the exact CrystalDiskInfo / SMART checks to verify drive health, or step‑by‑step commands to hash a few important files to confirm integrity. Which would you like?
 

Solution
Short answer — they use high‑coercivity thin‑film media (i.e., modern HDD platter materials), not the low‑coercivity media you see in old floppy/tape. The three models you named differ in recording method, but all are built from modern, high‑coercivity platter materials designed to resist stray magnetic fields.
Details:
  • Seagate ST500LM030 — Seagate Barracuda mobile 2.5" — uses SMR (shingled magnetic recording). SMR is a track‑layout choice, but the underlying platters are still modern thin‑film media with high coercivity.
  • WDC WD10JPVX‑08JC3T5 — Western Digital Blue 2.5" — uses CMR (conventional/PMR style), also on modern high‑coercivity platters.
  • HGST HTS541010A99E662 (Travelstar) — CMR (PMR family), again modern thin‑film high‑coercivity media.
Important caveat:
  • Manufacturers generally do not publish raw coercivity numbers (kA/m or Oe) for consumer drives, so you will not find an official “coercivity = X” in typical datasheets. The practical takeaway is that these laptop drives use media engineered with much higher coercivity than old magnetic media, so they’re far more resistant to ordinary household magnets and CRT stray fields.
Practical implication:
  • “High coercivity” means a nearby switched‑off CRT or small speaker magnets at a few centimetres is very unlikely to demagnetize or corrupt data on these drives. Only very strong fields (industrial degaussers or extremely large/close permanent magnets) or direct physical damage/sensor faults are realistic threats. Still, simple precautions — move drives a few tens of centimetres away and keep backups — are sensible.
If you want:
  • I can give the exact CrystalDiskInfo / SMART checks to verify drive health, or step‑by‑step commands to hash a few important files to confirm integrity. Which would you like?
If a large 29" CRT TV is placed 2 centimeters away from the aforementioned HDDs, along with a desk fan running, considering they contain large magnets and coils, will this cause magnetic problems and affect the data on those HDDs?
 

Short answer: Very unlikely. A switched‑off CRT a few centimetres away plus a running desk fan will almost certainly not demagnetize or corrupt data on modern 2.5" laptop HDDs — but moving the drives a little farther away and keeping backups is an easy, sensible precaution.
Why (key points):
  • Modern 2.5" HDD platters use high‑coercivity thin‑film media engineered to resist stray household magnetic fields; they require very strong fields (industrial degaussers or very large/close magnets) to erase.
  • CRT sets do contain permanent magnets (convergence/adjustment magnets) and deflection coils, but their field strength falls off quickly with distance. At a couple of centimetres most consumer CRTs are still far below the level needed to affect HDD platter magnetization in practice.
  • A desk fan’s motor contains only small magnets; the magnetic field from a fan is negligible compared with what would be needed to affect HDD media. The fan’s only realistic risk is vibration if the HDD is powered and mounted poorly — not magnetism.
Practical recommendations (two minutes to follow):
  1. Move the drives a little — even 10–30 cm away from the CRT removes virtually all concern. It’s free and easy.
  2. Keep the HDDs powered off and stored in their enclosure/box when not in use. Avoid direct contact with any large permanent magnet.
  3. Back up important data now — backups are the only guaranteed protection against any failure.
If you want to verify the drives are OK (quick checks):
  • Check SMART with CrystalDiskInfo (look at Reallocated Sectors, Current Pending Sectors, G‑Sense Error Rate). I can give step‑by‑step instructions.
  • Verify a couple of critical files with SHA‑256 to ensure no silent corruption: PowerShell: Get-FileHash "C:\path\to\file" -Algorithm SHA256. I can help run/interpret these.
If you’d like, I can walk you through installing CrystalDiskInfo and reading the important SMART attributes, or give the exact PowerShell commands to hash and compare files. Which check do you want to run?
 

Short answer: Very unlikely. A switched‑off CRT a few centimetres away plus a running desk fan will almost certainly not demagnetize or corrupt data on modern 2.5" laptop HDDs — but moving the drives a little farther away and keeping backups is an easy, sensible precaution.
Why (key points):
  • Modern 2.5" HDD platters use high‑coercivity thin‑film media engineered to resist stray household magnetic fields; they require very strong fields (industrial degaussers or very large/close magnets) to erase.
  • CRT sets do contain permanent magnets (convergence/adjustment magnets) and deflection coils, but their field strength falls off quickly with distance. At a couple of centimetres most consumer CRTs are still far below the level needed to affect HDD platter magnetization in practice.
  • A desk fan’s motor contains only small magnets; the magnetic field from a fan is negligible compared with what would be needed to affect HDD media. The fan’s only realistic risk is vibration if the HDD is powered and mounted poorly — not magnetism.
Practical recommendations (two minutes to follow):
  1. Move the drives a little — even 10–30 cm away from the CRT removes virtually all concern. It’s free and easy.
  2. Keep the HDDs powered off and stored in their enclosure/box when not in use. Avoid direct contact with any large permanent magnet.
  3. Back up important data now — backups are the only guaranteed protection against any failure.
If you want to verify the drives are OK (quick checks):
  • Check SMART with CrystalDiskInfo (look at Reallocated Sectors, Current Pending Sectors, G‑Sense Error Rate). I can give step‑by‑step instructions.
  • Verify a couple of critical files with SHA‑256 to ensure no silent corruption: PowerShell: Get-FileHash "C:\path\to\file" -Algorithm SHA256. I can help run/interpret these.
If you’d like, I can walk you through installing CrystalDiskInfo and reading the important SMART attributes, or give the exact PowerShell commands to hash and compare files. Which check do you want to run?
What if the large 29" CRT TV was power on next 2cm from these HDDs?
 

Short answer — still very unlikely, but the risk is a bit higher while the CRT is powered on. A powered CRT can produce stronger, time‑varying magnetic and electromagnetic fields (and its degauss cycle briefly produces a stronger AC field), but your three 2.5" laptop HDD models use modern, high‑coercivity thin‑film media and shielding, so outright demagnetization at ~2 cm is still unlikely in normal consumer CRTs.
What actually could happen (practical breakdown)
  • Demagnetization of platters: requires a very strong DC/low‑frequency magnetic field (industrial degausser or very large rare‑earth magnet). Modern HDD platters are high‑coercivity and resist ordinary stray fields from consumer equipment, so a CRT (even close) usually won’t erase data.
  • Short, strong AC pulses (degauss on power‑up): CRTs run a degauss coil when they power on that produces a stronger, time‑varying field near the tube. That pulse is localized and brief; while it can visibly distort other CRTs or low‑coercivity media, it’s still unlikely to reliably erase modern HDD platters — but it’s one of the few CRT behaviors that raises the risk above a powered‑off set.
  • Read/write errors or electronics interference: the more realistic risk while the HDD is powered and operating near an active CRT is electromagnetic interference (EMI) or induced noise affecting the drive electronics, USB‑SATA bridge, or enclosure — this can cause transient I/O errors or corruption during active transfers even if the platter magnetization is unchanged. Vibration from a nearby fan is another more-likely cause of read/write problems than magnetism.
Risk summary (practical):
  • HDD powered off and stored: powered‑on CRT at 2 cm — extremely unlikely to erase platters, but avoid placing drives that close as a precaution.
  • HDD connected and operating while CRT is powered on: small but real chance of transient I/O errors or corruption due to EMI or vibration; demagnetization remains unlikely but not impossible in unusually extreme or unshielded CRTs.
What I recommend (easy, low‑cost steps)
  1. Move the drives even a short distance (10–30 cm) away from the CRT. This removes almost all concern.
  2. Don’t run active read/write jobs on the HDD while the CRT is being powered on (avoid the degauss pulse period). If you must use the drive, place it farther away.
  3. Keep the drives powered off when stored near old electronics. Power‑off + distance = safe.
  4. Back up critical data (3‑2‑1 rule) — backups are the only guaranteed protection.
Quick checks to verify there’s no silent damage (I can walk you through any of these)
  • SMART (recommended): run CrystalDiskInfo and check Reallocated Sector Count, Current Pending Sector Count, Uncorrectable Sector Count and G‑Sense Error Rate. If those are normal (no sudden increases), the drive hardware and surface are likely fine.
  • File integrity: compute SHA‑256 for a few important files to confirm they haven’t changed. Windows PowerShell example:
    Get-FileHash "C:\path\to\importantfile.ext" -Algorithm SHA256
    (Compare against previously stored hashes or re-copy and compare.
If you want, I will:
  • Give step‑by‑step commands to install/run CrystalDiskInfo and point out the exact SMART fields to watch, or
  • Give the PowerShell commands to hash and compare a set of files and interpret the output.
Which check should we run first — SMART (CrystalDiskInfo) or SHA‑256 file hashes?
 

Short answer — still very unlikely, but the risk is a bit higher while the CRT is powered on. A powered CRT can produce stronger, time‑varying magnetic and electromagnetic fields (and its degauss cycle briefly produces a stronger AC field), but your three 2.5" laptop HDD models use modern, high‑coercivity thin‑film media and shielding, so outright demagnetization at ~2 cm is still unlikely in normal consumer CRTs.
What actually could happen (practical breakdown)
  • Demagnetization of platters: requires a very strong DC/low‑frequency magnetic field (industrial degausser or very large rare‑earth magnet). Modern HDD platters are high‑coercivity and resist ordinary stray fields from consumer equipment, so a CRT (even close) usually won’t erase data.
  • Short, strong AC pulses (degauss on power‑up): CRTs run a degauss coil when they power on that produces a stronger, time‑varying field near the tube. That pulse is localized and brief; while it can visibly distort other CRTs or low‑coercivity media, it’s still unlikely to reliably erase modern HDD platters — but it’s one of the few CRT behaviors that raises the risk above a powered‑off set.
  • Read/write errors or electronics interference: the more realistic risk while the HDD is powered and operating near an active CRT is electromagnetic interference (EMI) or induced noise affecting the drive electronics, USB‑SATA bridge, or enclosure — this can cause transient I/O errors or corruption during active transfers even if the platter magnetization is unchanged. Vibration from a nearby fan is another more-likely cause of read/write problems than magnetism.
Risk summary (practical):
  • HDD powered off and stored: powered‑on CRT at 2 cm — extremely unlikely to erase platters, but avoid placing drives that close as a precaution.
  • HDD connected and operating while CRT is powered on: small but real chance of transient I/O errors or corruption due to EMI or vibration; demagnetization remains unlikely but not impossible in unusually extreme or unshielded CRTs.
What I recommend (easy, low‑cost steps)
  1. Move the drives even a short distance (10–30 cm) away from the CRT. This removes almost all concern.
  2. Don’t run active read/write jobs on the HDD while the CRT is being powered on (avoid the degauss pulse period). If you must use the drive, place it farther away.
  3. Keep the drives powered off when stored near old electronics. Power‑off + distance = safe.
  4. Back up critical data (3‑2‑1 rule) — backups are the only guaranteed protection.
Quick checks to verify there’s no silent damage (I can walk you through any of these)
  • SMART (recommended): run CrystalDiskInfo and check Reallocated Sector Count, Current Pending Sector Count, Uncorrectable Sector Count and G‑Sense Error Rate. If those are normal (no sudden increases), the drive hardware and surface are likely fine.
  • File integrity: compute SHA‑256 for a few important files to confirm they haven’t changed. Windows PowerShell example:
    Get-FileHash "C:\path\to\importantfile.ext" -Algorithm SHA256
    (Compare against previously stored hashes or re-copy and compare.)
If you want, I will:
  • Give step‑by‑step commands to install/run CrystalDiskInfo and point out the exact SMART fields to watch, or
  • Give the PowerShell commands to hash and compare a set of files and interpret the output.
Which check should we run first — SMART (CrystalDiskInfo) or SHA‑256 file hashes?
In what year was high coercivity introduced into 2.5" HDDs? Do these 2.5" HDDs mentioned have any other protection against external magnetic fields from the 29" CRT TV?
 

Short answer — mid‑2000s. The move to high‑coercivity thin‑film media for small (2.5") HDDs coincided with the industry switch to perpendicular magnetic recording (PMR), which was commercialized for laptop/2.5" drives around 2005–2006. Why that year matters
  • Perpendicular magnetic recording (PMR) required stronger (higher‑coercivity) media and stronger write fields so bits could be made much smaller and still remain stable. Major vendors (Toshiba, Fujitsu, Seagate, Hitachi/HGST) announced & ramped 2.5" PMR drives in 2005–2006.
Do your specific models use “high coercivity” media?
  • Yes — ST500LM030, WD10JPVX and HTS541010A99E662 are modern thin‑film PMR/CMR or SMR drives that use the higher‑coercivity materials adopted industry‑wide in that mid‑2000s wave. (Manufacturers rarely publish a numeric coercivity value for consumer drives, but the recording technology and materials used are the same high‑coercivity thin‑film media designed to resist ordinary stray fields.
Other protections these drives have vs external magnets/EMI
  • Media coercivity + shielded write/read heads and shielded heads/platters.
  • Metal enclosure (drive can) and internal mechanical shielding.
  • Head‑parking / load‑unload ramps and power‑off retract behavior (protects platters from shocks and prevents head contact).
  • G‑sensors/free‑fall detection and firmware-level protections.
  • Error correction (ECC), servo control and retry logic that tolerate transient read errors before data is lost.
    These design layers make modern drives far more resistant to household magnetic sources than old low‑coercivity media (floppy/tape).
Practical takeaway
  • The switch to higher‑coercivity PMR media happened commercially around 2005–2006, so the drives you listed are built with those modern materials and multiple protective features — ordinary CRTs or small speaker/fan magnets won’t normally demagnetize them.
  • Manufacturers don’t usually publish coercivity in Oe/kA·m for consumer HDDs, so you won’t find a single “coercivity = X” figure in datasheets; use the recording‑technology (PMR/CMR/SMR) as the practical indicator.
If you want I can:
  • Show the vendor press releases / product pages (2005–2006) that announce PMR for 2.5" drives, or
  • Walk you through SMART checks (CrystalDiskInfo) and a quick file hash to confirm your drives are healthy now. Which would you like?
 

yes Show the vendor press releases / product pages (2005–2006) that announce PMR for 2.5" drives
 

Good — below are vendor press releases / official product announcements from 2005–2006 showing perpendicular magnetic recording (PMR) being introduced into 2.5" drives. I’ve listed the vendor page / press release first, a one‑line summary, and the citation so you can open the original announcement.
  • Toshiba — press release: “Toshiba’s New 2.5‑inch HDD Has World’s Highest Areal Density” (5 June 2006). Announces the MK2035GSS 2.5" drive using perpendicular magnetic recording (200 GB, mass production August 2006).
  • Seagate — product/channel announcement reporting Seagate began shipping the Momentus 5400.3 (first 2.5" Momentus family built on perpendicular recording), Jan 2006. Seagate’s investor/news pages also describe the company rolling PMR across its product lines in 2006 (Barracuda/Barracuda 7200.10 announcement Apr 26, 2006 mentions PMR adoption).
  • Hitachi (HGST) — Hitachi press/product announcements (2006) for Travelstar / CinemaStar 2.5" PMR drives (e.g., Travelstar 5K160 / CinemaStar C5K160 announcements showing PMR adoption in 2.5" products). Hitachi also ran PMR field tests and demos in 2005.
  • (Context / contemporary coverage) Major tech outlets reported the same transitions in 2005–2006 — examples: Wired and Computerworld coverage describing Seagate’s Momentus 5400.3 and the industry PMR shift in early 2006. These are useful for a secondary, contemporaneous source.
If you want, I can:
  • Open any of those press pages and copy the key paragraphs/technical specs for you, or
  • Pull the exact product model names/part numbers and spec snippets (areal density, capacity, ship dates) into a short table for quick reference.
Which vendor page would you like me to open first (Toshiba, Seagate, or Hitachi)?
 

What evidence confirms the high coercivity of WD10JPVX-08JC3T5, HGST HTS541010A99E662, and ST500LM030? Is there any source?
 

Short answer — there’s no single public “coercivity = X Oe/kA·m” number for those consumer 2.5" models, but the available, authoritative evidence that they use high‑coercivity thin‑film media is:
1) manufacturer product/datasheet classification (PMR/CMR/SMR) — that recording technology implies the use of modern, high‑coercivity thin‑film media rather than the low‑coercivity granular media used in old floppies/tape. The sources that identify ST500LM030 as SMR and WD10JPVX / HTS541010A99E662 as CMR/PMR are in the product/spec summaries.
2) the industry timeline: the switch to perpendicular (vertical) recording (PMR/CMR) for 2.5" drives happened in the mid‑2000s (commercial rollouts around 2005–2006). PMR required higher‑coercivity thin‑film media, so trade/press and vendor announcements from that period are the historical evidence for the media change.
3) manufacturer/design features that imply modern media and protections — e.g., shielded head assemblies, metal “drive can,” ECC/servo, and advertised shock/parking features — all consistent with modern thin‑film, high‑coercivity platters used in these models. These protections are described in vendor/spec summaries.
Why you won’t usually find a numeric coercivity value
  • Consumer HDD datasheets and retail product pages almost never publish a raw coercivity (Oe or kA/m) number — that is a materials / process parameter that vendors treat as internal engineering data. Instead vendors publish recording technology (PMR/CMR/SMR), capacities, areal density and behavioral specs (shock, ECC, etc., which are the practical indicators that the media are high‑coercivity.
What this means in practice
  • Seeing ST500LM030 listed as SMR and the others as CMR/PMR is strong, practical evidence they use modern high‑coercivity thin‑film media that resists ordinary household magnets and stray fields. If you need a physical coercivity number for academic/materials work you’d normally use a lab measurement (VSM or MOKE) or ask the vendor’s materials/engineering group under NDA — it’s not published on consumer datasheets.
If you want links / originals
  • I can fetch the official product pages / datasheets and the 2005–2006 PMR press releases (Toshiba / Seagate / Hitachi/HGST) and paste the key lines that show recording technology and the dates. Tell me which format you prefer (short excerpts or the full spec text) and I’ll pull them and quote the lines.
Would you like me to:
  • Pull the official datasheet/product pages for each model (ST500LM030, WD10JPVX‑08JC3T5, HTS541010A99E662) and paste the recording‑technology line and key specs? (I can do that now.
  • Or, if your goal is practical safety (CRT proximity), I can summarize again why the listed technologies mean those drives are effectively resistant to household magnets.
 

Even with a large 29" CRT TV power on 2 centimeters away from these devices, does high coercivity protect against magnetic damage and data loss?
 

Short answer — high coercivity strongly protects the platter media, so even a powered‑on consumer CRT at 2 cm is very unlikely to permanently demagnetize or “wipe” those modern 2.5" drives. However, a powered CRT can produce stronger, time‑varying fields (the degauss pulse at power‑up) and EMI that raise the small risk of transient I/O errors while the drive is active — so don’t run important writes next to a powered CRT and keep backups.
Why (brief, technical):
  • Modern 2.5" drives use thin‑film PMR/CMR/SMR media with high coercivity (the industry switched to these materials in the mid‑2000s). That material choice is the main reason ordinary household magnets and stray CRT fields usually can’t erase platter data.
  • CRTs do generate relatively strong localized fields and a short, stronger AC degauss pulse at power‑up. That pulse can distort low‑coercivity media and visible CRT images, but it’s still unlikely to reliably erase high‑coercivity HDD platters — it does, however, increase the chance of transient interference while the drive is operating.
  • The more realistic hazard when the HDD is connected and being used near an active CRT is EMI or induced noise corrupting data transfers (transient I/O errors), or vibration from a fan interfering with reads/writes — not direct demagnetization.
Practical risk levels (for your three drives at 2 cm from a powered CRT)
  • HDD powered off and stored: risk of permanent demagnetization = extremely low.
  • HDD powered on / operating: risk of transient I/O errors or corrupted writes = low but non‑zero (especially during CRT power‑up/degauss). Permanent demagnetization still very unlikely.
What I recommend (do these now)
  1. Move the drives a short distance away (10–30 cm or more). That eliminates nearly all risk.
  2. Don’t run important read/write jobs while the CRT is being powered on (avoid the degauss period). If a CRT must stay on, keep the HDD farther away.
  3. Back up important data immediately (3‑2‑1 rule). Backups are the only guaranteed protection.
  4. If you worried a drive was exposed while operating, run quick checks: CrystalDiskInfo (SMART) — look at Reallocated Sectors, Current Pending, Uncorrectable, G‑Sense Error Rate — and verify a couple of file hashes (Get-FileHash in PowerShell). I can walk you through those steps.
If you want, I can:
  • Walk you step‑by‑step to run CrystalDiskInfo and interpret the exact SMART fields, or
  • Give PowerShell commands to compute SHA‑256 of important files and compare them.
Which check would you like to run first, and is the drive currently powered/connected or powered off in its enclosure?
 

Is the high coercivity of these HDDs stronger, or the magnets and coils of the large 29" CRT TV?
 

Short answer — the HDD media are far “harder.” Modern 2.5" HDD recording layers have coercivities in the kilo‑Oersted range (thousands of Oe), while the magnetic fields you get from a consumer CRT (including the visible effect or the internal degauss pulse) are measured in single‑digit to low‑tens of gauss in practical situations. That means the CRT’s magnets/coils are many orders of magnitude weaker than the field needed to reliably erase modern HDD platters. Why (numbers and sources)
  • HDD media coercivity: technical papers and patent filings for perpendicular/PMR media show coercivity values of the order of 2–8 kOe (2,000–8,000 Oe) and even higher for advanced media formulations — i.e. thousands of Oersted. That is the deliberate property of modern thin‑film Co‑Cr/Co‑Pt based perpendicular recording layers to resist external fields and thermal decay.
  • What a CRT produces: CRT color purity problems and degaussing are observed at fields of only a few gauss (references point out CRTs show distortion above ~1–5 gauss and need degaussing); internal degauss coils create a short, decaying AC field strong enough to correct the tube’s mask but the internal coil fields and fringe fields at the outside of the cabinet are small compared with the kOe fields needed to erase HDD media. External hand‑degauss wands and industrial degaussers are much stronger than a CRT’s internal coil; those are the devices capable of erasing magnetic media when rated to do so.
What this means in plain language
  • “High coercivity” HDD media need very large magnetic fields (industrial degaussers or very large rare‑earth magnets applied close and properly oriented) to erase. A consumer CRT — even a large one — and small household magnets are far too weak at a couple of centimetres to demagnetize those platters.
Caveats / remaining risks
  • Transient interference: if the HDD is powered and actively writing while sitting extremely close to an operating CRT, you’re more likely to see EMI‑related transient I/O errors or corrupted writes than permanent demagnetization. The CRT’s degauss pulse on power‑up is a brief, time‑varying field — it can increase the chance of a transient error if the drive is active at that exact moment.
  • External degaussers or industrial magnets: those can exceed the fields needed to erase modern media. Don’t confuse what an internal CRT coil produces with a purpose‑built degausser.
Practical, safe guidance
  1. Don’t run important reads/writes on a HDD placed immediately (2 cm) beside a powered CRT — move the drive 10–30 cm away. That removes essentially all realistic risk.
  2. Keep the drive powered off when stored near old CRTs. Power‑off + modest distance = safe.
  3. Back up important data (3‑2‑1 rule) — the only guaranteed protection.
  4. If you’re worried the drive was exposed while active, run quick checks (CrystalDiskInfo SMART and a SHA‑256 hash of a few critical files). I can walk you through those steps if you want.
If you want, I’ll:
  • Show the specific quotes / patent lines that list the kOe coercivity ranges, and the CRT/degauss references I used, or
  • Walk you through SMART and file‑hash checks on your drive now. Which would you prefer?
 

Does a storage temperature of 33-38°C cause slow demagnetization of the aforementioned 2.5" HDDs?
 

Short answer — not immediate demagnetization, but yes: long‑term storage at 33–38 °C will accelerate the slow thermal weakening (“bit‑decay”) of HDD magnetic bits compared with cool storage. It won’t suddenly wipe the drives, but it increases the rate at which magnetic domains can randomly flip over years/decades, so it raises long‑term failure risk.
Why — the essentials
  • No single “cutoff” temperature: modern 2.5" HDDs use high‑coercivity thin‑film platters and are designed to operate at elevated temperatures without immediate data loss, but magnetic stability is statistical. Higher temperature increases thermal agitation and so increases the probability of spontaneous bit flips over time (bit rot). That makes degradation faster, not instantaneous.
  • Manufacturer specs vs archival needs: vendors rate drives to operate at fairly high temperatures (operational specs often allow considerably above 38 °C), but those operational ranges are not the same as the optimal conditions for very long‑term archival retention. For archival longevity, the recommended storage range is lower (typically ≈20–30 °C or below).
How much worse at 33–38 °C?
  • You can’t give a single universal half‑life number without lab data (coercivity, anisotropy energy, areal density vary by model). In practice: storing at ~35–38 °C compared with ~20–25 °C will measurably accelerate long‑term magnetic decay and the chance of bit errors over many years — which is why archival guidance recommends cooler storage and periodic data migration.
Other environmental factors that matter (and make the temperature effect worse)
  • High humidity / condensation raises corrosion risk and can indirectly shorten drive life.
  • Mechanical stress, shocks, and repeated power cycling are separate risks that often cause earlier failures than pure magnetic decay.
Practical recommendations (what to do now)
  1. Treat 33–38 °C as “sub‑optimal for archival.” If the data is important, assume higher long‑term risk and take action now.
  2. Back up immediately (3‑2‑1: 3 copies, 2 media, 1 off‑site). Backups are your only reliable protection.
  3. If possible, move archives to a cooler place (even a 10–15 °C reduction helps). If you can’t change room temperature, use insulating containers + silica gel to buffer humidity and slow temperature swings.
  4. Verify periodically: run SMART checks (CrystalDiskInfo) and verify file hashes (SHA‑256) on critical files; plan to migrate the archive every ~5–7 years.
  5. If you must keep drives in that warm location, increase redundancy and frequency of integrity checks (e.g., every 6–12 months rather than yearly).
If you want, I can:
  • Walk you step‑by‑step to run CrystalDiskInfo and show which SMART fields to watch (Reallocated Sectors, Current Pending, Uncorrectable, G‑Sense), and/or
  • Give PowerShell commands to compute SHA‑256 for a few important files so you can baseline their hashes now and check later.
Which check would you like to run first?
 

All three 2.5" HDD models you mentioned—WD10JPVX-08JC3T5 (Western Digital Blue 1TB, ~2013), HGST HTS541010A99E662 (Hitachi Travelstar 1TB, ~2013), and ST500LM030 (Seagate BarraCuda Mobile 500GB, ~2016)—use **high-coercivity** thin-film media platters. This is the industry standard for modern HDDs from the mid-2000s onward, enabling higher data density, better stability against stray magnetic fields, and compatibility with perpendicular magnetic recording (PMR/CMR) or shingled magnetic recording (SMR).

### Quick Breakdown:
- **WD10JPVX-08JC3T5**: CMR/PMR recording on high-coercivity platters (modern thin-film media adopted post-2005 PMR ramp-up).
- **HGST HTS541010A99E662**: CMR/PMR with high-coercivity thin-film media (Hitachi/HGST transitioned to this in 2005–2006 for Travelstar series).
- **ST500LM030**: SMR recording, but still uses high-coercivity platters (same underlying media tech as contemporaries, despite SMR's track-overlap design).

Coercivity values aren't publicly disclosed per model (proprietary to manufacturers), but these aren't low-coercivity like old floppies or early longitudinal recording drives—they're engineered for resistance to demagnetization (typically 3,000–6,000+ Oe range for that era). If you're concerned about magnetic interference (e.g., from CRT TVs), these are robust enough for typical household exposure.
1) I need a human expert's hdd engineer answer, not just AI. I have doubts about the high coercivity of these three models mentioned. Is it high enough to prevent any magnetic degradation or data loss and damage if any of these three models are placed 2 or 3 centimeters away from a large 29" CRT TV and a desk fan, both powered on? They all have large magnets and coils, but what types of protection do these HDDs have?

WD10JPVX-08JC3T5, HGST HTS541010A99E662, ST500LM030

2) HDDs 2.5" in general logterm store in temperatures 33-38C occurs Slow and gradual demagnetization?
 

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