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Solar Bulletin, May 2003
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 59 Number 5 | May 2003 |
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Table I. Mean Sunspot Numbers for May 2003 [boldface = maximum, minimum] | Table II. May Observers |
| Day |
N |
Raw |
s.d. |
Ra |
s.d. |
s.e. |
| 1 |
38 |
149 |
7.0 |
105 |
2.4 |
0.39 |
| 2 |
42 |
130 |
8.2 |
93 |
3.2 |
0.49 |
| 3 |
46 |
128 |
6.5 |
94 |
2.5 |
0.37 |
| 4 |
57 |
131 |
5.2 |
98 |
2.1 |
0.28 |
| 5 |
36 |
126 |
6.1 |
94 |
2.9 |
0.48 |
| 6 |
34 |
104 |
5.0 |
77 |
2.7 |
0.46 |
| 7 |
44 |
72 |
4.1 |
55 |
2.6 |
0.39 |
| 8 |
37 |
44 |
3.0 |
31 |
1.6 |
0.26 |
| 9 |
49 |
27 |
1.1 |
21 |
0.7 |
0.10 |
| 10 |
52 |
25 |
1.0 |
19 |
0.7 |
0.10 |
| 11 |
47 |
41 |
2.0 |
30 |
1.0 |
0.15 |
| 12 |
42 |
56 |
2.7 |
41 |
1.5 |
0.23 |
| 13 |
39 |
60 |
2.9 |
43 |
1.2 |
0.19 |
| 14 |
40 |
59 |
2.8 |
44 |
1.3 |
0.21 |
| 15 |
40 |
65 |
3.4 |
47 |
1.6 |
0.25 |
| 16 |
38 |
64 |
2.7 |
47 |
1.4 |
0.23 |
| 17 |
48 |
51 |
2.8 |
39 |
1.4 |
0.20 |
| 18 |
48 |
59 |
3.3 |
42 |
1.6 |
0.23 |
| 19 |
46 |
80 |
4.3 |
58 |
2.1 |
0.31 |
| 20 |
36 |
81 |
4.6 |
58 |
2.3 |
0.38 |
| 21 |
42 |
76 |
3.9 |
55 |
1.9 |
0.29 |
| 22 |
38 |
85 |
4.4 |
60 |
2.3 |
0.37 |
| 23 |
35 |
71 |
6.1 |
51 |
2.9 |
0.49 |
| 24 |
39 |
47 |
3.5 |
34 |
1.6 |
0.26 |
| 25 |
39 |
57 |
3.1 |
42 |
1.7 |
0.27 |
| 26 |
39 |
80 |
5.4 |
57 |
2.1 |
0.34 |
| 27 |
45 |
77 |
4.2 |
58 |
2.0 |
0.30 |
| 28 |
51 |
85 |
4.8 |
63 |
2.1 |
0.29 |
| 29 |
49 |
82 |
4.1 |
60 |
1.6 |
0.23 |
| 30 |
51 |
64 |
2.6 |
47 |
1.0 |
0.14 |
| 31 |
40 |
59 |
3.0 |
42 |
1.1 |
0.17 |
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Means: | 42.8 | 75.3 | | 55.1 | | |
No. of Observations: 1327
No. of Observers: 79
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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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| 10 |
AAP |
P.Abbott |
| 27 |
ARAG |
G.Araujo |
| 19 |
ATON |
A.Attanasio |
| 15 |
BARH |
H.Barnes |
| 14 |
BATR |
R.Battaiola |
| 21 |
BERJ |
J.Berdejo |
| 9 |
BLAJ |
J.Blackwell |
| 10 |
BMF |
M.Boschat |
| 23 |
BOJP |
P.Bojda |
| 26 |
BOSB |
B.Bose |
| 31 |
BRAB |
B.Branchett |
| 21 |
BRAD |
D.Branchett |
| 18 |
BRAR |
R.Branch |
| 27 |
BROB |
R.Brown |
| 3 |
BURS |
S.Burgess |
| 8 |
CAMP |
P.Campbell |
| 14 |
CARJ |
J.Carlson |
| 30 |
CHAG |
G.Morales |
| 29 |
CKB |
B.Cudnik |
| 9 |
CLZ |
C.Laurent |
| 10 |
COMT |
T.Compton |
| 31 |
CORA |
A.Coroas |
| 22 |
CR |
T.Cragg |
| 8 |
CVJ |
J.Carvajal |
| 28 |
DEJV |
J.van Delft |
| 6 |
DELS |
S.Delaney |
| 5 |
DEMF |
F.Dempsey |
| 16 |
DGP |
G.Dyck |
| 24 |
DRAJ |
J.Dragesco |
| 28 |
DUBF |
F.DuBois |
| 28 |
ELR |
E.Reed |
| 11 |
FEEC |
C.Feehrer |
| 19 |
FERJ |
J.Fernandes |
| 25 |
FLET |
T.Fleming |
| 18 |
FUJK |
K.Fujimori |
| 20 |
GIOR |
R.Giovanoni |
| 23 |
GOEM |
M.Goetz |
| 3 |
GOLA |
A.Golovin |
| 10 |
GOTS |
S.Gottschalk |
| 5 |
HALB |
B.Halls |
| 8 |
HAYK |
K.Hay |
| 2 |
HUZR |
R.Huziak |
| 18 |
JAMD |
D.James |
| 10 |
JEFT |
T.Jeffrey |
| 7 |
JENJ |
J.Jenkins |
| 22 |
KAPJ |
J.Kaplan |
| 21 |
KHAR |
R.Khan |
| 22 |
KNJS |
J&S Knight |
| 2 |
KROL |
L.Krozel |
| 5 |
KUZM |
M.Kuzmin |
| 10 |
LARJ |
J.Larriba |
| 12 |
LERM |
M.Lerman |
| 18 |
LEVM |
M.Leventhal |
| 21 |
MALK |
K.Malde |
| 29 |
MARJ |
J.Maranon |
| 19 |
MCE |
E.Mochizuki |
| 2 |
MILJ |
J.Miller |
| 15 |
MMI |
M.Moeller |
| 16 |
OBSO |
IPS Observatory |
| 7 |
PARN |
N.Parker |
| 14 |
RICE |
E.Richardson |
| 17 |
RITA |
A.Ritchie |
| 5 |
SCHG |
G.Scholl |
| 12 |
SIMC |
C.Simpson |
| 24 |
STAB |
B.Gordon-States |
| 14 |
STEF |
G.Stefanopoulis |
| 26 |
STEM |
G.Stemmler |
| 26 |
STQ |
N.Stoikidis |
| 22 |
SUZM |
M.Suzuki |
| 23 |
SZUM |
M.Szulc |
| 25 |
TESD |
D.Teske |
| 8 |
THR |
R.Thompson |
| 14 |
TJV |
J.Temprano |
| 26 |
URBP |
P.Urbanski |
| 19 |
VARG |
A.Vargas |
| 9 |
VELM |
M.Velea |
| 26 |
VIDD |
D.Vidican |
| 19 |
WILW |
W.Wilson |
| 28 |
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 2003 |
| Day |
RG |
S:G |
Day |
RG |
S:G |
Day |
RG |
S:G |
Day |
RG |
S:G |
| 1 |
7.3 |
10.4 |
9 |
2.2 |
2.3 |
17 |
3.4 |
5.0 |
25 |
3.5 |
6.3 |
| 2 |
6.1 |
11.3 |
10 |
2.1 |
1.9 |
18 |
3.6 |
6.4 |
26 |
4.2 |
9.1 |
| 3 |
6.4 |
10.0 |
11 |
3.3 |
2.4 |
19 |
4.4 |
8.2 |
27 |
3.8 |
10.3 |
| 4 |
6.5 |
10.2 |
12 |
4.5 |
2.4 |
20 |
4.6 |
7.6 |
28 |
4.4 |
9.3 |
| 5 |
6.8 |
8.5 |
13 |
4.2 |
4.3 |
21 |
4.6 |
6.5 |
29 |
4.3 |
9.1 |
| 6 |
6.3 |
6.5 |
14 |
4.1 |
4.4 |
22 |
6.0 |
4.2 |
30 |
3.3 |
9.4 |
| 7 |
4.9 |
4.7 |
15 |
4.7 |
3.8 |
23 |
5.5 |
2.9 |
31 |
3.3 |
7.9 |
| 8 |
3.5 |
2.6 |
16 |
4.6 |
3.9 |
24 |
3.8 |
2.4 |
Mn. |
4.5 |
6.3 |
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Click image to enlarge. Fig.1. 10 cm Solar Flux and Comparison of Ri (provisional) and Ra Estimates for May 2003 (r=0.981).
(Ri Source: http://sidc..oma.be/index.php3)
(10cm Source: http://www.drao.nrc.ca/icarus) |
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Click image to enlarge. Fig.2 Maximum, Mean, and Minimum Ra Values for Each Month from January 2001 to Present. |
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 2003
| (Analysis performed by Michael Hill, SID Analyst) |
| Date |
Max |
Imp |
Date |
Max |
Imp |
Date |
Max |
Imp |
| Date |
Max |
Imp |
Date |
Max |
Imp |
Date |
Max |
Imp |
| 030501 |
1141 |
1 |
030526 |
0551 |
2+ |
030531 |
1534 |
1 |
| 030501 |
1414 |
1+ |
030526 |
1513 |
1+ |
030531 |
1631 |
1+ |
| 030501 |
1922 |
2 |
030526 |
1522 |
2 |
030531 |
1641 |
2 |
| 030502 |
0307 |
2 |
030526 |
1637 |
2 |
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| 030502 |
1816 |
3+ |
030527 |
0349 |
2+ |
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| 030502 |
1831 |
2+ |
030527 |
0623 |
2+ |
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| 030503 |
0951 |
1- |
030527 |
1506 |
2+ |
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| 030503 |
1832 |
1+ |
030527 |
1513 |
2+ |
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| 030504 |
0813 |
1- |
030527 |
2307 |
2 |
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| 030504 |
1351 |
1- |
030528 |
0025 |
3 |
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| 030504 |
1507 |
1- |
030528 |
0610 |
2+ |
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| 030506 |
1014 |
2 |
030528 |
1425 |
1 |
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| 030506 |
1403 |
2+ |
030528 |
1546 |
1+ |
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| 030506 |
1410 |
2 |
030528 |
1733 |
1+ |
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| 030506 |
1921 |
2 |
030528 |
1746 |
1+ |
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| 030507 |
0617 |
1 |
030528 |
1805 |
1- |
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| 030507 |
0711 |
1+ |
030528 |
1847 |
2 |
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| 030507 |
1028 |
1 |
030528 |
1939 |
1 |
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| 030507 |
1057 |
1- |
030529 |
0105 |
2 |
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| 030507 |
1312 |
1 |
030529 |
0220 |
1+ |
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| 030507 |
2032 |
1- |
030529 |
1936 |
2 |
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| 030507 |
2049 |
2 |
030530 |
0651 |
1+ |
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| 030507 |
2139 |
1+ |
030530 |
0921 |
1 |
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| 030508 |
0554 |
2+ |
030531 |
0225 |
2+ |
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| 030522 |
0700 |
2+ |
030531 |
1417 |
1 |
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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 |
| W Sharlack |
A09 |
NAA |
| A Clerkin |
A29 |
NAA |
| J Winkler |
A50 |
NAA NPM NPR |
| D Toldo |
A52 |
NWC |
| A Panzer |
A83 |
NAA |
| M Hill |
A87 |
NAA |
| L Anderson |
A91 |
NWC |
| G DiFillipo |
A93 |
DHO |
| T Poulos |
A95 |
NAA |
| R Battaiola |
A96 |
DHO |
| J Wallace |
A97 |
NAA |
| M King |
A99 |
HWU |
| P Campbell |
A100 |
NLK |
| G Bressan |
A101 |
DHO |
| F Steyn |
A102 |
NAA NWC |
| L Observatory |
A107 |
DHO |
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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 was not an overly active month but it sure got busy towards the end. There were only 53 reported SID events this month, none of them having an importance rating greater than 2+. The middle of the month from the 10th to the 20th had very little activity, if any, on any given day. There was a short active period around the 20th and then the sun became very active on the 25th and remained this way until the end of the month. The GOES-10 Satellite measured only 159 X-Ray events. Of these, only eight were M-Class; however, there were 3 X-Class flares. All three of them were centered on the 28th, which was the most active day indeed. Along with the X-Class flare that occurred that day, there were also 16 C-Class flares as well.
The sun has been keeping things interesting and with these large sunspot groups that continue to emerge as the cycle progesses, things may, in fact, remain that way for the time being. So I hope you all have your systems working optimally and are able to record these interesting bursts of activity that we keep seeing once or twice a month. Thanks to all of you for sumitting data so regularly. I want to thank all of you as well for making your sumittals of data promtly after the end of the month. This is very helpful to me.
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