Morphology and Spectral Behavior of Solar Hard X-Ray Sources
Images of 17 solar flares, corresponding to 61 individual X-ray bursts observedin four energy bands (14-23, 23-33, 33-53, and 53-93 keV) by the Hard X-RayTelescope (HXT) experiment aboard the Yohkoh satellite have been investigated.The images suggest that the angular size of the hard X-ray sources i...
I tiakina i:
| I whakaputaina i: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Ngā kaituhi matua: | , |
| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
Universidad Nacional Autónoma de México
2002
|
| Ngā marau: | |
| Urunga tuihono: | https://www.redalyc.org/articulo.oa?id=57138201 |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
|