Home Page
About Us Page
Links Page
Contact Us Page
Forums Page
Users Pages
Guestbook Page
Search Site Page
Project Page
 
Home | Profile | Active Topics | Active Polls | Search | FAQ
Username:
 Password:
Save Password
Forgot your Password?

 All Forums
 Main Area
 General Chatter Area
 More C-flares are possible,probability for an M-fl

Note: You must be registered in order to post a reply.

Screensize:
UserName:
Password:
Format Mode:
Format: BoldItalicizedUnderlineStrikethrough Align LeftCenteredAlign Right Horizontal Rule Insert HyperlinkInsert EmailInsert Image Insert CodeInsert QuoteInsert List Spell Checker
   
Message:
* HTML is OFF
* Forum Code is ON
Smilies
Smile [:)] Big Smile [:D] Cool [8D] Blush [:I]
Tongue [:P] Evil [):] Wink [;)] Clown [:o)]
Black Eye [B)] Eight Ball [8] Frown [:(] Shy [8)]
Shocked [:0] Angry [:(!] Dead [xx(] Sleepy [|)]
Kisses [:X] Approve [^] Disapprove [V] Question [?]

  Check here to include your profile signature.
 Check here to subscribe to this topic.
    

T O P I C    R E V I E W
vk3pa Posted - 22 Mar 2006 : 07:47:45 AM
Catania sunspot group 15 (NOAA AR 0862) has grown up further
and developed a beta-gamma configuration of the photospheric magnetic
field. C2.5 and C1.3 flares (peaking at 09:44 UT and 12:04 UT
respectively) occurred today in this group. More C-flares are possible,
and there is a low probability for an M-flare. The solar wind speed
decreased down to around 600 km/s and the magnetic field remains at the
average level. We expect quiet geomagnetic conditions for the next 48
hours.

Goldfields DX Amateur Radio Group © 2002 - 2022 Goldfields DX Amateur Radio Group Go To Top Of Page
This page was generated in 0.56 seconds. Snitz Forums 2000