Birdwatch Note
2024-03-09 07:49:24 UTC - MISINFORMED_OR_POTENTIALLY_MISLEADING
You need a hydrogen-alpha filter(H-alpha). H-alpha filters pass a narrow wavelength of light centered on the H-alpha emission line of hydrogen (656.28 nm), This wavelength is where solar flares, filaments, prominences, and other dynamic features are more visible. https://www.astronomy.com/science/how-to-choose-a-hydrogen-alpha-filter/
Written by DE66E4120DA09A101328409E18B6DC3DB338213C89BAB618D82854E1419E1A9F
Participant Details
Original Tweet
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All Information
- ID - 1766370688384827467
- noteId - 1766370688384827467
- participantId -
- noteAuthorParticipantId - DE66E4120DA09A101328409E18B6DC3DB338213C89BAB618D82854E1419E1A9F Participant Details
- createdAtMillis - 1709970564349
- tweetId - 1766249294888161660
- classification - MISINFORMED_OR_POTENTIALLY_MISLEADING
- believable -
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- summary
- You need a hydrogen-alpha filter(H-alpha). H-alpha filters pass a narrow wavelength of light centered on the H-alpha emission line of hydrogen (656.28 nm), This wavelength is where solar flares, filaments, prominences, and other dynamic features are more visible. https://www.astronomy.com/science/how-to-choose-a-hydrogen-alpha-filter/
Note Status History
| createdAt | timestampMillisOfFirstNonNMRStatus | firstNonNMRStatus | timestampMillisOfCurrentStatus | currentStatus | timestampMillisOfLatestNonNMRStatus | mostRecentNonNMRStatus | participantId |
| 2024-03-09 07:49:24 UTC (1709970564349) |
2024-03-09 13:49:18 UTC (1709992158047) |
CURRENTLY_RATED_HELPFUL | 2024-03-10 02:46:15 UTC (1710038775311) |
CURRENTLY_RATED_HELPFUL | 2024-03-09 13:49:18 UTC (1709992158047) |
CURRENTLY_RATED_HELPFUL |
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