OT - Other
2019-01-01T02:00:09 -> 2019-01-01T11:00:09
xcen, ycen = 1005,576
Description: It is not clear whether this represents a mass ejection, but the origin and development of the concave structure seems to be a mystery. The phenomenon is specific to the 171 A channel. A better view may be obtained by PROBA-2/SWAP (174 A) and GOES/SUVI (171 A) with larger fields of view.
Solar Object Locator:
| SOL2019-01-01T02:00:09L296C061 |
Properties:
| Event Title | Formation and slow detachment of a large concave structure |
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Data Source
| Observatory | SDO |
|---|---|
| Instrument | AIA |
| Mean Wavelength | 1.710e-06 cm |
| Channel ID | 171 |
Rating:
| Overall Rating | 3.0 (0=lowest, 5=highest) |
|---|---|
| Number of Ratings | 1 |
Identification Method
| FRM Name | halocme (Other features and events submitted by halocme) |
|---|---|
| FRM Institute | LMSAL |
| FRM Contact | Scott Green |
| FRM Date Run | 2019-01-05T21:31:20 |
| FRM Identifier | Annotator-20171220-ext |
| FRM Parameters | n/a |
| FRM URL | n/a |
| FRM Human Flag | true |
Nearby Events:
| View in iSolSearch |
| Get SDO Data |
References:
| Movie | |
|---|---|
| HER VOEvent | XML |
| Full HER VOEvent |
| First Event IVORN | Edge Type | Second Event IVORN | Strength | Reported By |
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Revisions:
| Revision # | Revision Date | Revised By |
|---|---|---|
| 1 | 2019-01-05 | nitta_nariaki |
Comments:
| Comment By | Comment Date | Comment |
|---|