RAID 0 Data Recovery Services
RAID 0 splits data across two or more drives with no redundancy. When any member fails, the entire array goes offline, and every file in the volume is affected. Our RAID data recovery service handles RAID 0 arrays by imaging every member through write-blocked channels, repairing dead drives at the board level when needed, and reconstructing the stripe pattern offline from cloned images. Free evaluation. No data, no charge.

What Makes RAID 0 Recovery Different from Other RAID Levels?
RAID 0 is the only common RAID level with zero fault tolerance. A single member failure makes the entire volume inaccessible because every file's data is distributed across all drives with no parity or mirror copy to fill gaps.
- RAID 1 mirrors data, so one healthy member contains everything. RAID 5 uses distributed parity to tolerate one member loss. RAID 6 tolerates two. RAID 0 tolerates none. Every member must be readable for recovery to succeed.
- Data is written in fixed-size stripes (blocks) that alternate across members. A two-drive RAID 0 with a 128KB stripe size writes the first 128KB to Drive 0, the next 128KB to Drive 1, the next to Drive 0, and so on. A 500MB file on a two-member array has roughly 250MB of its blocks on each drive.
- This striping architecture means a dead member does not just remove some files; it removes alternating chunks of every file. Without that member's stripe blocks, the filesystem cannot be parsed and individual files cannot be assembled.
- RAID 0 is common in video editing workstations, gaming rigs, scratch disks for large renders, and older NAS configurations built for throughput over safety. Users choose it for raw sequential read/write speed and full capacity utilization (no space is consumed by parity or mirroring).
- The recovery challenge is twofold: first, every member must be successfully imaged. Second, the stripe size and member order must be detected from raw data, since there is no parity information to help validate the configuration.
Why Can Dead RAID 0 Members Still Be Recovered?
Some data recovery labs declare RAID 0 arrays unrecoverable the moment any member drive stops responding. Rossmann Group handles these arrays by repairing failed members at the component level before imaging.
- A drive that will not spin, clicks on power-up, or shows no electrical response is not necessarily destroyed. Common causes include burned TVS diodes from power surges, failed motor driver ICs, seized spindle motors, and degraded head stack assemblies. Each of these has a defined repair path.
- PCB-level failures are diagnosed using diode-mode measurements, thermal imaging, and microscope inspection. Failed components are identified and replaced at the individual IC level. We do not swap entire donor boards, which often fails because modern drives store adaptive calibration data in PCB ROM that is unique to each head-platter combination.
- Head swaps are performed in a 0.02 micron ULPA-filtered clean bench. Donor heads are sourced from matching model and firmware revision drives. After transplant, the drive is connected to PC-3000 imaging hardware for write-blocked cloning.
- Seized spindle motors are addressed through motor transplants, where the platters are moved to a functional donor motor assembly under laminar flow conditions. Platter alignment is verified before imaging begins.
- The repair serves one purpose: making the member readable long enough to complete a full sector-by-sector clone. Once all members are imaged, the array can be reconstructed in software regardless of the original drives' condition.
Our RAID 0 Recovery Process
We follow a six-step image-first workflow: evaluate the array, clone every member through write-blocked hardware, repair any non-responsive drives, detect stripe parameters, reconstruct the volume offline, and extract files from the clone.
- Free evaluation and configuration mapping: Document the array layout: number of members, controller type (hardware RAID card, motherboard RAID, or software RAID via mdadm/Windows Dynamic Disks), original stripe size if known, and slot positions. No work is performed on original drives during evaluation.
- Write-blocked forensic imaging of every member: Each member is connected to PC-3000 or DeepSpar imaging hardware through write-blocked channels. Conservative retry profiles and head-maps are configured per drive to maximize read coverage while minimizing surface stress. Every sector is cloned to a target image before any reconstruction begins.
- Board-level repair for non-responsive members: Members that fail to spin, click on power-up, or show electrical faults are diagnosed at the component level. Burned TVS diodes, failed motor drivers, and damaged preamplifier circuits are repaired via micro-soldering. Head swaps and motor transplants are performed in a 0.02 micron ULPA-filtered clean bench. The goal is to make the drive readable long enough to complete a full clone.
- Stripe parameter detection and member ordering: Specialized virtual assembly software tests stripe sizes (64KB, 128KB, 256KB, and others) against the cloned images. It identifies the correct block size by finding the configuration that produces contiguous filesystem structures. Member order is determined by analyzing where partition tables, boot sectors, and filesystem superblocks land across the stripe sequence.
- Virtual array assembly and filesystem extraction: The array is reconstructed virtually from cloned images using the detected stripe size and member order. Filesystem structures (NTFS, EXT4, XFS, HFS+) are parsed from the reconstructed volume. Files are extracted, verified against expected types, and copied to your target media.
- Delivery and secure purge: Recovered data is transferred to your supplied drive or new media. File listings are reviewed with you to confirm priority data is intact. All working copies are securely purged on request.
How Stripe Size and Member Order Are Detected
RAID 0 arrays store no parity data that could help validate parameters. Stripe size and member sequence must be determined by analyzing raw data patterns across the cloned member images.
- RAID controllers use a configurable stripe (block) size, commonly 64KB, 128KB, or 256KB, though some controllers allow 4KB through 1MB. This value determines how much contiguous data is written to one member before the controller moves to the next.
- Virtual assembly software performs automated stripe-size detection by testing each candidate block size against the member images. The correct size produces a recognizable partition table and filesystem superblock at the expected offsets in the reconstructed stream.
- Member order (which physical drive maps to logical position 0, 1, 2, etc.) is determined by examining where known structures appear. A GPT partition table, for example, starts at LBA 1. On a RAID 0 array, whichever member holds the first stripe block containing LBA 1 is member 0 in the stripe sequence.
- Hardware RAID cards (Dell PERC, LSI MegaRAID, Adaptec) often store metadata in a reserved region at the start or end of each member disk. When this metadata survives, it provides the stripe size, member order, and array UUID directly, avoiding brute-force detection.
- Software RAID implementations (Windows Dynamic Disks, Linux mdadm) store superblocks at known offsets on each member. These superblocks record stripe size, member count, array UUID, and member position, simplifying reconstruction when the superblocks are intact.
How Much Does RAID 0 Recovery Cost?
RAID 0 recovery is priced per member (each drive in the array) plus an array reconstruction fee. If we recover nothing, you owe $0.
- Per-member imaging reflects the condition of each individual drive, not the RAID level. A healthy drive with firmware corruption costs less than a drive needing a head swap.
- The array reconstruction fee covers stripe parameter detection, virtual assembly, and filesystem extraction from the reconstructed volume.
Per-Member Imaging
- Logical or firmware-level issues: From $250 to $600–$900 per drive. Covers filesystem corruption, firmware module damage requiring PC-3000 terminal access, and SMART threshold failures that block normal reads.
- Mechanical failures (head swap, motor seizure): $1,200–$1,500 per drive with a 50% deposit. Donor parts are consumed during the transplant. Head swaps and platter work are performed on a validated laminar-flow bench before write-blocked cloning with DeepSpar imaging hardware.
Array Reconstruction
- $400-$800 depending on member count, stripe complexity, filesystem type (NTFS, EXT4, XFS, HFS+), and whether parameters must be detected from raw data or can be read from surviving RAID metadata.
- UFS Explorer and R-Studio perform parameter detection, virtual assembly, and filesystem-level extraction from cloned member images after the drives are safely imaged.
No Data = No Charge: If we recover nothing from your array, you owe $0. Free evaluation, no obligation.
Example: A two-drive RAID 0 where both members have firmware corruption would cost From $250 to $600–$900 per drive plus $400-$800 for reconstruction.
Where RAID 0 Arrays Are Most Common
RAID 0 is used wherever raw throughput and full capacity matter more than fault tolerance. The tradeoff is accepted because the data is either backed up elsewhere or considered replaceable.
Video editing workstations
Timeline playback of 4K and 6K footage requires sustained sequential read speeds that a single drive cannot provide. RAID 0 stripes reads across members, multiplying throughput. The source footage typically lives on a separate archive or LTO tape.
Scratch and render disks
3D rendering, scientific simulation, and database staging generate large temporary files. RAID 0 provides the write speed needed for intermediate output. The final results are copied to redundant storage after the job completes.
Gaming and performance arrays
Consumer motherboards with onboard RAID support encourage RAID 0 for faster game load times and application launches. These arrays contain no parity and are often the user's only copy of the data.
How Is Chunk Size Determined in a Failed RAID 0 Array?
Chunk size is found by testing candidate sizes against cloned member images until filesystem boundaries align across the stripe set. Virtual assembly software automates this search using NTFS MFT spacing or ext4 inode-table spacing as validation signals.
RAID 0 stripes data across members in fixed-size chunks. Common sizes are 64 KB, 128 KB, 256 KB, 512 KB, and 1 MB. When controller metadata is lost, the chunk size is unknown and must be rediscovered before virtual assembly.
For NTFS arrays, the Master File Table stores 1,024-byte FILE records at predictable intervals. If we assume a 128 KB chunk size and the MFT records line up contiguously across members at that boundary, the assumption is validated. If they do not, we test the next candidate.
For ext4 arrays, the inode table has fixed spacing based on superblock parameters. The ext4 magic value is 0xEF53, stored as bytes 53 EF at offset 0x438. From this filesystem start, we calculate the data_offset. Once the offset is known, inode table alignment across members reveals the chunk size.
- Chunk size
- The fixed data segment written to each member before the controller advances to the next disk in the stripe set.
- Stripe size
- The total width of a single stripe row: chunk size multiplied by the number of data-bearing members.
- Filesystem boundary analysis
- Using known filesystem structure spacing (MFT, inode tables, boot sector repetition) to validate a guessed chunk size against cloned images.
How Is Disk Order Reconstructed Without Parity Data?
Disk order is reconstructed by signature solving, tracing a file header larger than the stripe width across member images, followed by heuristic permutation verification. Hardware RAID cards store disk order in trailing-sector metadata; mdadm stores it in the superblock.
RAID 0 has no parity. Without parity stripes to use as anchors, you cannot simply solve for missing data. But you can solve for sequence. The method is signature solving: locate a file (JPEG header, ZIP local-file-header, or PDF magic bytes) that is larger than the stripe width. The file header will span multiple members in the correct order. By mapping the header fragments across the cloned images, we determine which member holds position 0, position 1, and so on.
Heuristic verification then brute-forces the remaining disk-order permutations. For each permutation, the virtual array is assembled and the filesystem coherence is scored: Are directory entries valid? Do MFT record sequences increment logically? Does the ext4 block group descriptor checksum match? The permutation with the highest score is the correct disk order.
In practice, hardware RAID controllers make this easier. Dell PERC and LSI MegaRAID write the disk sequence into trailing-sector DDF metadata. HP Smart Array stores equivalent geometry in a proprietary RAID Information Sector near the start of each drive. We read that metadata directly from the member images. mdadm Linux software RAID stores member position in the mdadm superblock: version 0.90 at the end of the device, 1.0 at 8-12 KB from the end, 1.1 at byte offset 0, or 1.2 at 4 KB from the start. If the superblock is intact, disk order is explicit.
- Image every member drive to a raw binary clone.
- Search for known file signatures that exceed the stripe width.
- Map signature fragments across members to establish initial sequence.
- Brute-force remaining permutations and score filesystem coherence.
- Validate against controller trailing-sector metadata or mdadm superblock if present.
Is RAID 0 Data Recovery Actually Possible?
Yes. RAID 0 recovery is feasible when every member can be imaged before further damage. The myth that RAID 0 is unrecoverable persists because labs that cannot repair dead drives in-house declare the case lost when a single member fails mechanically.
You have probably heard that RAID 0 data is gone forever if one drive dies. The engineering reality is more nuanced. RAID 0 stripes data without parity. If one member is completely unresponsive and cannot be imaged even after board-level repair or head-stack replacement, then any file that spans the missing member is partial or lost. But files smaller than the chunk size that live entirely on the surviving members are intact. And if the dead member can be repaired and imaged, the full stripe set can be reconstructed.
The actual workflow is straightforward. First, image every member drive individually. Consumer drives are rated at roughly one Unrecoverable Read Error per 10^14 bits read, which is approximately 12.5 TB. A long, continuous imaging pass on aging multi-terabyte drives can encounter UREs. We image with ddrescue or PC-3000 Express to handle bad sectors without hanging the source drive.
Second, detect the array parameters, including chunk size, disk order, and data offset, from trailing-sector metadata or filesystem analysis. Third, assemble the array virtually from the disk images. Fourth, extract the filesystem and verify files against known signatures.
Competitors who say RAID 0 is impossible usually lack the equipment to repair the member hardware. They do not have a 0.02 micron ULPA-filtered clean bench for head swaps. They do not have PC-3000 Express for firmware-level imaging. They do not have Hakko FM-2032 microsoldering stations for PCB repair. When the member drive is mechanically dead, their only option is to declare the case unrecoverable. We fix the drive first, then recover the data.
How Does RAID 0 Compare to RAID 1, RAID 5, and RAID 6 for Fault Tolerance?
RAID 0 has zero fault tolerance. It carries no parity and no mirror, so any single member loss takes the whole volume offline. RAID 1 keeps a full mirror, RAID 5 holds one XOR parity block per stripe, and RAID 6 holds dual P+Q parity, so each of those survives at least one member failure where RAID 0 survives none.
| RAID Level | Fault Tolerance | Minimum Members | Usable Capacity Efficiency | Single-Member-Loss Outcome | Recovery Approach |
|---|---|---|---|---|---|
| RAID 0 | 0 drives. No redundancy. | 2 | 100% (no capacity spent on parity or mirror) | Whole volume offline. Every striped file loses its blocks on the dead member. | Repair and image the dead member, then reconstruct stripe geometry virtually. No parity equation exists to recompute missing blocks. |
| RAID 1 | 1 drive (n-1 in a multi-way mirror) | 2 | 50% (two-way mirror) | Array stays online. A surviving mirror member holds a full copy. | Image a healthy mirror member directly; no stripe assembly required. |
| RAID 5 | 1 drive (single XOR parity) | 3 | (n-1)/n | Array runs degraded on parity. A second member failure exceeds tolerance; a URE during rebuild aborts on legacy controllers, while modern controllers puncture the affected stripe. | For the irreplaceable, unbacked, degrading case, image every member first and reconstruct virtually from clones rather than rebuilding live on marginal hardware. |
| RAID 6 | 2 drives (dual P+Q parity) | 4 | (n-2)/n | Array stays online with one member down; tolerates a second failure during rebuild. | Image every member, then solve P and Q parity virtually against the clones to fill any gaps. |
The RAID 5 and RAID 6 rows carry a caveat the RAID 0 row cannot. Consumer drives carry a worst-case manufacturer spec of about one URE per 10^14 bits read (~12.5 TB), which is a warranty floor rather than a schedule, so a long degraded RAID 5 rebuild on large aging members raises the probability of hitting an unreadable sector. What happens then depends on the controller: legacy and low-end controllers abort and drop the volume, while modern Dell PERC and LSI/Broadcom MegaRAID puncture the stripe, write a bad-block placeholder, and finish the rebuild with only that stripe lost. For the irreplaceable, unbacked, degrading case we image RAID 5 and RAID 6 member by member first, then reconstruct the array offline. RAID 0 has no parity and no rebuild: it has neither XOR parity nor P+Q, so a URE corrupts the affected file rather than failing a parity calculation, and a member failure destroys the volume outright with no parity block to recompute anything.
- Fault tolerance
- The number of member drives that can fail while the array still serves data. RAID 0 tolerates zero; RAID 1 and RAID 5 tolerate one; RAID 6 tolerates two.
- XOR parity
- The single parity block RAID 5 computes per stripe by XOR-ing the data blocks in that stripe. A missing data block is recomputed by XOR-ing the surviving blocks with the parity block. RAID 0 stores no parity, so this recomputation is not available.
- P+Q dual parity
- RAID 6 stores two independent syndromes per stripe: P (an XOR sum) and Q (a Reed-Solomon code). The two syndromes let RAID 6 solve for up to two missing members in a stripe. RAID 0 has no equivalent.
How Do RAID 0 Striping Mechanics Affect Data Recovery?
RAID 0 distributes every file across all members in fixed chunks with no parity, so a permanently lost member leaves gaps in every file that spanned it. There is no equation to solve for the missing blocks, which forces one of two paths: physically repair and image the dead member, or carve only files that landed entirely on surviving members.
- Confirm whether the dead member is repairable. With no XOR parity (RAID 5) and no Reed-Solomon P+Q (RAID 6) to fall back on, a missing member's blocks cannot be recomputed. Repairing and imaging that member is the only path to a complete reconstruction.
- Image every surviving member to a raw clone through write-blocked hardware before any assembly. Reconstruction runs against the clones, never against the live drives.
- Establish chunk size and member order from the clones so the surviving data lines up at the correct stripe offsets.
- If the dead member is imaged, assemble the full stripe set virtually and extract the filesystem. If it is not, fall back to carving files that fit within the contiguous run on the surviving members.
The chunk size sets a hard ceiling on what partial carving can recover when one member is permanently lost. In a two-member RAID 0, only the chunks that landed on the surviving member are intact. A file is fully recoverable from a single survivor only if it fits inside one contiguous chunk on that member. With a 64 KB chunk, that ceiling is small; with a 1 MB chunk, more whole files happen to land on one member, but anything larger than a chunk still loses the alternating blocks the dead member held. Larger chunk sizes raise the partial-carve yield, they do not make spanning files whole.
This is the structural difference from a parity array. RAID 5 and RAID 6 can reconstruct a missing member's blocks arithmetically from the surviving members and their parity. RAID 0 holds no parity at all, so the surviving members carry no information about the missing chunks. That is why dead-member repair, not arithmetic, is the deciding factor in RAID 0 outcomes.
RAID 0 Recovery Questions
Can you recover a RAID 0 if one drive is completely dead?
How do you determine the stripe size of a RAID 0 array?
Is partial recovery possible if one RAID 0 member cannot be imaged?
What is the difference between RAID 0 and JBOD?
How long does RAID 0 recovery take?
What happens if the RAID 0 superblock is wiped?
Can hardware RAID 0 arrays be recovered without the original controller?
Why do some labs say RAID 0 is unrecoverable?
Data Recovery Standards & Verification
Our Austin lab operates on a transparency-first model. We use industry-standard recovery tools, including PC-3000 and DeepSpar, combined with strict environmental controls to maintain drive integrity. This approach allows us to serve clients nationwide with consistent technical standards.
Open-drive work is performed in a ULPA-filtered laminar-flow bench, validated to 0.02 µm particle count, verified using TSI P-Trak instrumentation.
Transparent History
Serving clients nationwide via mail-in service since 2008. Our lead engineer holds PC-3000 and HEX Akademia certifications for hard drive firmware repair and mechanical recovery.
Media Coverage
Our repair work has been covered by The Wall Street Journal and Business Insider, with CBC News reporting on our pricing transparency. Louis Rossmann has testified in Right to Repair hearings in multiple states and founded the Repair Preservation Group.
Aligned Incentives
Our "No Data, No Charge" policy means we assume the risk of the recovery attempt, not the client.
Technical Oversight
Louis Rossmann
Our engineers review all lab protocols to maintain technical accuracy and honest service. Since 2008, his focus has been on clear technical communication and accurate diagnostics rather than sales-driven explanations.
We believe in proving standards rather than just stating them. We use TSI P-Trak instrumentation to verify that clean-air benchmarks are met before any drive is opened.
See our clean bench validation data and particle test videoNeed your RAID 0 array recovered?
Free evaluation. No data = no charge. Mail-in from anywhere in the U.S.