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Solar Bulletin, May 2005
Solar Bulletin |
| THE AMERICAN ASSOCIATION OF VARIABLE STAR OBSERVERS - SOLAR COMMITTEE |
Carl E. Feehrer, Editor
9 Gleason Rd.
Bedford, MA 01730 | Email: cfeehrer@hotmail.com
ISSN 0271-8480 |
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| Volume 61 Number 5 | May 2005 |
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Table I. Mean Sunspot Numbers for May 2005 [boldface = maximum, minimum] | Table II. May Observers
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| Day |
N |
Raw Mean |
Ra |
| 1 |
37 |
52 |
38 |
| 2 |
40 |
51 |
37 |
| 3 |
42 |
62 |
44 |
| 4 |
35 |
58 |
42 |
| 5 |
43 |
57 |
40 |
| 6 |
37 |
56 |
42 |
| 7 |
36 |
51 |
35 |
| 8 |
42 |
59 |
43 |
| 9 |
38 |
80 |
57 |
| 10 |
40 |
106 |
75 |
| 11 |
35 |
109 |
77 |
| 12 |
33 |
101 |
73 |
| 13 |
26 |
85 |
60 |
| 14 |
32 |
72 |
51 |
| 15 |
29 |
57 |
41 |
| 16 |
32 |
57 |
39 |
| 17 |
30 |
43 |
31 |
| 18 |
33 |
29 |
20 |
| 19 |
37 |
25 |
18 |
| 20 |
38 |
16 |
11 |
| 21 |
27 |
20 |
13 |
| 22 |
32 |
30 |
21 |
| 23 |
37 |
32 |
22 |
| 24 |
35 |
35 |
24 |
| 25 |
43 |
42 |
30 |
| 26 |
47 |
55 |
38 |
| 27 |
46 |
57 |
40 |
| 28 |
34 |
54 |
36 |
| 29 |
38 |
59 |
42 |
| 30 |
28 |
62 |
42 |
| 31 |
37 |
70 |
49 |
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Means: | 36.1 | 56.2 | 39.7 |
No. of Observers: 62
No. of Observations: 1119
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Reporting Addresses |
Sunspot Reports -- email: solar@aavso.org
- postal mail: AAVSO, 25 Birch St. Cambridge, MA 02138
- FAX (AAVSO): (617) 354-0665
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SID Solar Flare Reports -- email: noatak@aol.com
- postal mail: Mike Hill
114 Prospect St. Marlboro, MA 01752
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|
| 16 |
AAP |
P.Abbott |
| 26 |
ARAG |
G.Araujo |
| 2 |
ARE |
R.Allessi |
| 7 |
BARH |
H.Barnes |
| 19 |
BATR |
R.Battaiola |
| 16 |
BEB |
R.Berg |
| 14 |
BERJ |
J.Berdejo |
| 2 |
BLAJ |
J.Blackwell |
| 9 |
BMF |
M.Boschat |
| 19 |
BOSB |
B.Bose |
| 25 |
BRAB |
B.Branchett |
| 29 |
BRAR |
R.Branch |
| 22 |
BROB |
R.Brown |
| 27 |
BVK |
K.Bankston |
| 30 |
CHAG |
G.Morales |
| 31 |
CKB |
B.Cudnik |
| 12 |
CLZ |
L.Corp |
| 12 |
COMT |
T.Compton |
| 28 |
CR |
T.Cragg |
| 20 |
DEJV |
J.van Delft |
| 6 |
DEMF |
F.Dempsey |
| 25 |
DRAJ |
J.Dragesco |
| 27 |
DUBF |
F.Dubois |
| 2 |
FEEC |
C.Feehrer |
| 21 |
FERJ |
J.Fernandez |
| 24 |
FLET |
T.Fleming |
| 24 |
FUJK |
K.Fujimori |
| 17 |
GOEM |
M.Goetz |
| 12 |
HAYK |
K.Hay |
| 17 |
HRUT |
T.Hrutkay |
| 24 |
JAMD |
D.James |
| 8 |
JENJ |
J.Jenkins |
| 19 |
KAPJ |
J.Kaplan |
| 29 |
KNJS |
J&S |
| 2 |
KROL |
L.Krozel |
| 9 |
LARJ |
J.Larriba |
| 10 |
LERM |
M.Lerman |
| 20 |
LEVM |
M.Leventhal |
| 18 |
MARE |
E.Mariani |
| 29 |
MARJ |
J.Maranon |
| 25 |
MCE |
E.Mochizuki |
| 5 |
MEU |
E.Mason |
| 11 |
MMI |
M.Moeller |
| 19 |
OBSO |
IPS Observatory |
| 13 |
RICE |
E.Richardson |
| 10 |
RITA |
A.Ritchie |
| 25 |
SCGL |
G.Schott |
| 10 |
SCHG |
G.Scholl |
| 14 |
SIMC |
C.Simpson |
| 6 |
STEF |
G.Stefanopoulis |
| 19 |
STEM |
G.Stemmler |
| 25 |
STQ |
N.Stoikidis |
| 25 |
SUZM |
M.Suzuki |
| 26 |
SZAK |
K.Szatkowski |
| 26 |
SZUM |
M.Szulc |
| 7 |
THR |
R.Thompson |
| 25 |
TJV |
J.Temprano |
| 27 |
URBP |
P.Urbanski |
| 21 |
VARG |
A.Vargas |
| 17 |
VIDD |
D.Vidican |
| 27 |
WILW |
W.Wilson |
| 27 |
YESH |
H.Yesilyaprak |
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| Table III. Means of Raw Group Counts (RG) and Ratios of Spots to Groups (S:G) in May 2005 |
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Click image to enlarge. Fig. 1. 10 cm Solar Flux and American Relative Sunspot Numbers (Ra) for May 2005
(10cm Source: http://www.drao.nrc.ca/icarus) |
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Click image to enlarge. Fig.2 Smoothed Mean Sunspot Numbers (Waldmeier method) from January 2000 to November 2004. |
Michael Hill, SID Analyst
114 Prospect St
Marlborough, MA 01752 USA
noatak@aol.com |
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Sudden Ionospheric Disturbances (SID) Recorded During May 2005
| (Analysis performed by Michael Hill, SID Analyst) |
| Date |
Max |
Imp |
Date |
Max |
Imp |
Date |
Max |
Imp |
| 050501 |
0019 |
1- |
050511 |
1930 |
1+ |
050518 |
0829 |
1+ |
| 050501 |
0820 |
1- |
050511 |
1943 |
2+ |
050521 |
1351 |
2+ |
| 050501 |
1637 |
2+ |
050512 |
0116 |
1- |
050526 |
2109 |
1+ |
| 050503 |
1037 |
1+ |
050512 |
0702 |
1 |
050526 |
2136 |
2 |
| 050505 |
1444 |
1+ |
050512 |
0734 |
2 |
050527 |
0508 |
1- |
| 050505 |
2019 |
1+ |
050512 |
1357 |
2+ |
050527 |
0635 |
1+ |
| 050506 |
0317 |
2+ |
050512 |
1707 |
1 |
050527 |
1231 |
2+ |
| 050506 |
0552 |
2+ |
050512 |
1743 |
2+ |
050528 |
0231 |
2 |
| 050506 |
1127 |
2 |
050512 |
1954 |
1- |
050528 |
0500 |
1- |
| 050507 |
0812 |
2 |
050513 |
0822 |
1+ |
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| 050507 |
0851 |
1- |
050513 |
1643 |
2+ |
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| 050509 |
1104 |
2 |
050513 |
1709 |
2 |
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| 050509 |
1147 |
1+ |
050514 |
1507 |
1+ |
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| 050509 |
1233 |
1+ |
050514 |
1601 |
1+ |
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| 050509 |
2107 |
2+ |
050515 |
1748 |
2+ |
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| 050510 |
0523 |
2+ |
050515 |
1856 |
2+ |
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| 050510 |
0907 |
1+ |
050515 |
2046 |
1 |
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| 050510 |
1227 |
1 |
050515 |
2236 |
2 |
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| 050510 |
1838 |
1+ |
050516 |
0242 |
1+ |
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| 050510 |
1952 |
1+ |
050516 |
0911 |
2 |
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| 050510 |
1959 |
2 |
050516 |
1301 |
1+ |
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| 050511 |
0623 |
1- |
050517 |
0240 |
1+ |
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| 050511 |
0643 |
2+ |
050517 |
0404 |
1 |
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| 050511 |
0908 |
1+ |
050517 |
0553 |
1+ |
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| 050511 |
1702 |
1+ |
050517 |
1021 |
2+ |
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| Importance rating: Duration | -1: <19 | 1: 19-25 | 1+: 26-32 | 2: 33-45 | 2+: 46-85 | 3: 86-125 | 3+: >125 |
| Observer |
Code |
Station(s) monitored |
| A Clerkin |
A29 |
NAA NAU |
| J Winkler |
A50 |
NAA NML NPM |
| D Toldo |
A52 |
NWC XXX |
| W Moos |
A84 |
ICV |
| M Hill |
A87 |
NAA |
| J Mandaville |
A90 |
NPM |
| L Anderson |
A91 |
NWC |
| G Di Filippo |
A93 |
HWU |
| T Poulos |
A95 |
NAA |
| R Battaiola |
A96 |
HWU |
| J Wallace |
A97 |
NAA |
| M King |
A99 |
HWU |
| F Steyn |
A102 |
NAA NWC |
| B Bose |
A103 |
VTX |
| L Observatory |
A107 |
DHO |
| P Mortfield |
A108 |
NAA |
| M Suhovecky |
A115 |
NAA |
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| The events listed above meet at least one of the following criteria |
- Event reported by two or more observers within +/- 5 minutes
- Event matched to GOES-8 XRA event to within +/- 15 minutes and event time < 1000 UT
- Reported by observer with a high quality rating > 8 (scale 1-10)
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May turned out to be a fairly active month for SID events. As opposed to last month's mere twelve events, this month we recorded 60 correlated SID events. The GOES-12 satellite recored 221 X-Ray flares and of these, 13 were M-Class events with the peak activity being around the beginning of the month and mid-month.
The SID event count actually surprised me at first because although a number of you had lengthy reports, none approached this number. The maximum number of events reported by any one observer was 29. The reason the count was so high however was the good coverage across the entire day provided by our network of observers, which runs from California to Massachussets, across the Atlantic to England, Switzerland, Italy, Greece, South Africa, India, and Australia. This coverage is very important and all of you in all the corners of the world serve an important function to capture all the SID events which this month, more than others I have seen, were spread quite evenly across the 24 hours of the day on all the active days. The results of this month point to the strength of our network and the importance of each and every one of you to make it that way. Keep up the good work and thanks to all.
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Solar Flare Summary Based on GOES-12 Data
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