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
 : We are experiencing active solar conditions, pos

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 - 07 Jul 2006 : 06:42:32 AM
COMMENT: We are experiencing active solar conditions, possibly leading
to geomagnetic disturbances. This morning an M2.5 long duration event
(LDE) was recorded by GOES.
Its start-peak-end times are
08:11-08:37-08:58 UT and it is still decaying. A post-eruptive arcade
(PEA) and dimmings near the active region are visible in EIT, and the
associated CME appeared at 08:54 UT in LASCO C2. We roughly estimate the
CME speed to be higher than 500 km/s. The CME itself seems to erupt to
the SW, nevertheless we can expect some geomagnetic disturbance from it
within 3 days.
The high energy proton fluxes (>10MeV and >30MeV) are
enhanced from 9 UT onwards, but didn't reach the proton event threshold.
As the active region is turning near the west limb we have set a warning
condition for proton events
.
At present geomagnetic conditions are again quiet, after the
active-minor storm interval induced by the transequatorial coronal hole.
The solar wind speed is still elevated at 600 km/s, but the IMF
intensity remains low around 4nT with a weak and oscillating Bz
component.

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