M is for Magnifique Part Deux
From RHESSI Wiki
(Difference between revisions)
(Created page with "{{Infobox Nugget |name = Nugget |title = M is for Magnifique |number = 146 |first_author = Steven Christe |second_author = Andy Inglis |publish_date = 21 February 2011 |next_nugg...") |
m |
||
Line 11: | Line 11: | ||
== Introduction == | == Introduction == | ||
- | In this nugget, we would like to continue our analysis of the M class flare of October 16th 2010 (SOL2010-10-16T19:12) which we have previously discussed in a [M is for Magnifique|past nugget]. | + | In this nugget, we would like to continue our analysis of the M class flare of October 16th 2010 (SOL2010-10-16T19:12) which we have previously discussed in a [[M is for Magnifique|past nugget]]. |
+ | |||
+ | == CMEs == | ||
+ | |||
+ | Such a moving shock front might be indicative of a CME. | ||
+ | |||
+ | [[File:2010oct16_GBSRBSradio.png|thumb|center|600px|'''Figure X''': The radio spectrum from GBSRBS showing associated type III and type II radio bursts. Type II radio bursts are signatures of traveling shock waves and are frequently associated with CMEs.]] | ||
+ | |||
+ | |||
== Conclusion == | == Conclusion == |
Revision as of 21:30, 8 February 2011
Nugget | |
---|---|
Number: | 146 |
1st Author: | Steven Christe |
2nd Author: | Andy Inglis |
Published: | 21 February 2011 |
Next Nugget: | |
Previous Nugget: | [At last, the EUV Spectrum] |
List all |
Introduction
In this nugget, we would like to continue our analysis of the M class flare of October 16th 2010 (SOL2010-10-16T19:12) which we have previously discussed in a past nugget.
CMEs
Such a moving shock front might be indicative of a CME.
Conclusion
Facts about M is for Magnifique Part DeuxRDF feed
RHESSI Nugget Date | 21 February 2011 + |
RHESSI Nugget First Author | Steven Christe + |
RHESSI Nugget Index | 146 + |
RHESSI Nugget Second Author | Andy Inglis + |