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Solar Bulletin, November 2004
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 60 Number 11 | November 2004 |
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Table I. Mean Sunspot Numbers for November 2004 [boldface = maximum, minimum] | Table II. November Observers
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| Day |
N |
Raw Mean |
Ra |
| 1 |
25 |
106 |
79 |
| 2 |
21 |
121 |
81 |
| 3 |
29 |
95 |
70 |
| 4 |
29 |
79 |
60 |
| 5 |
34 |
82 |
61 |
| 6 |
40 |
97 |
71 |
| 7 |
37 |
93 |
68 |
| 8 |
26 |
88 |
62 |
| 9 |
31 |
76 |
55 |
| 10 |
27 |
49 |
35 |
| 11 |
24 |
49 |
36 |
| 12 |
26 |
57 |
43 |
| 13 |
33 |
61 |
47 |
| 14 |
35 |
71 |
53 |
| 15 |
24 |
59 |
45 |
| 16 |
28 |
63 |
45 |
| 17 |
26 |
61 |
43 |
| 18 |
27 |
49 |
36 |
| 19 |
22 |
46 |
33 |
| 20 |
24 |
49 |
35 |
| 21 |
28 |
36 |
28 |
| 22 |
21 |
40 |
31 |
| 23 |
26 |
41 |
30 |
| 24 |
28 |
51 |
39 |
| 25 |
24 |
51 |
38 |
| 26 |
28 |
53 |
40 |
| 27 |
26 |
55 |
40 |
| 28 |
22 |
46 |
32 |
| 29 |
29 |
41 |
32 |
| 30 |
26 |
46 |
35 |
| 31 |
--- |
--- |
--- |
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Means: | 27.5 | 63.7 | 46.7 |
No. of Observers: 57
No. of Observations: 826
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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 |
| 4 |
ARE |
R.Allessi |
| 8 |
BARH |
H.Barnes |
| 6 |
BATR |
R.Battaiola |
| 8 |
BEB |
R.Berg |
| 9 |
BERJ |
J.Berdejo |
| 12 |
BMF |
M.Boschat |
| 8 |
BOSB |
B.Bose |
| 26 |
BRAB |
B.Branchett |
| 25 |
BRAR |
R.Branch |
| 24 |
BROB |
R.Brown |
| 3 |
CAMP |
P.Cambell |
| 30 |
CHAG |
G.Morales |
| 13 |
CKB |
B.Cudnik |
| 12 |
CLZ |
L.Corp |
| 9 |
COMT |
T.Compton |
| 29 |
CR |
T.Cragg |
| 24 |
DEJV |
J.van Delft |
| 5 |
DGP |
G.Dyck |
| 2 |
DPP |
P.dePonthiere |
| 20 |
DRAJ |
J.Dragesco |
| 11 |
DUBF |
F.Dubois |
| 10 |
FEEC |
C.Feehrer |
| 12 |
FERJ |
J.Fernandez |
| 14 |
FLET |
T.Fleming |
| 25 |
FUJK |
K.Fujimori |
| 9 |
HAYK |
K.Hay |
| 5 |
HRUT |
T.Hrutkay |
| 18 |
JAMD |
D.James |
| 17 |
KAPJ |
J.Kaplan |
| 26 |
KNJS |
J&S Knight |
| 12 |
KROL |
L.Krozel |
| 13 |
LARJ |
J.Larriba |
| 21 |
LEVM |
M.Leventhal |
| 5 |
MARE |
E.Mariani |
| 22 |
MARJ |
J.Maranon |
| 24 |
MCE |
E.Mochizuki |
| 12 |
MEU |
E.Mason |
| 17 |
MMI |
M.Moeller |
| 20 |
OBSO |
IPS Observatory |
| 6 |
RICE |
E.Richardson |
| 22 |
RITA |
A.Ritchie |
| 14 |
SCGL |
G.Schott |
| 6 |
SIMC |
C.Simpson |
| 4 |
STEF |
G.Stefanopoulis |
| 9 |
STEM |
G.Stemmler |
| 20 |
STQ |
N.Stoikidis |
| 23 |
SUZM |
M.Suzuki |
| 17 |
SZUM |
M.Szulc |
| 17 |
TESD |
D.Teske |
| 12 |
THR |
R.Thompson |
| 12 |
TJV |
J.Temprano |
| 12 |
URBP |
P.Urbanski |
| 13 |
VARG |
A.Vargas |
| 10 |
WILW |
W.Wilson |
| 22 |
YESH |
H.Yesilyaprak |
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| Table III. Means of Raw Group Counts (RG) and Ratios of Spots to Groups (S:G) in November 2004 |
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Click image to enlarge. Fig. 1. 10 cm Solar Flux and American Relative Sunspot Numbers (Ra) for November 2004
(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 May 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 November 2004
| (Analysis performed by Michael Hill, SID Analyst) |
| Date |
Max |
Imp |
Date |
Max |
Imp |
Date |
Max |
Imp |
| 041101 |
0704 |
2 |
041105 |
1921 |
2+ |
041109 |
0629 |
2 |
| 041102 |
0145 |
1 |
041106 |
0029 |
1 |
041109 |
0741 |
1- |
| 041102 |
0943 |
1+ |
041106 |
0150 |
2 |
041109 |
0747 |
2 |
| 041102 |
0949 |
1+ |
041106 |
0657 |
1 |
041109 |
0923 |
1- |
| 041102 |
1400 |
1 |
041106 |
1432 |
1 |
041109 |
1053 |
1- |
| 041103 |
0132 |
1+ |
041106 |
1548 |
1- |
041109 |
1435 |
2+ |
| 041103 |
0336 |
2+ |
041106 |
1600 |
1+ |
041109 |
1715 |
2 |
| 041103 |
0902 |
1- |
041106 |
1608 |
1+ |
041109 |
1802 |
1 |
| 041103 |
0909 |
1 |
041106 |
1656 |
1- |
041110 |
0211 |
2 |
| 041103 |
1348 |
1- |
041106 |
1714 |
1+ |
041110 |
0734 |
1 |
| 041103 |
1547 |
2 |
041106 |
1953 |
2 |
041110 |
0814 |
2 |
| 041103 |
1642 |
1 |
041106 |
2101 |
1 |
041112 |
0955 |
2 |
| 041103 |
1654 |
1- |
041107 |
0146 |
1+ |
041118 |
1457 |
1- |
| 041103 |
1818 |
2+ |
041107 |
0419 |
2 |
041119 |
0051 |
1- |
| 041103 |
1827 |
3 |
041107 |
0452 |
1+ |
041119 |
0514 |
2+ |
| 041104 |
0904 |
2 |
041107 |
0801 |
1 |
041123 |
0852 |
1+ |
| 041104 |
2059 |
2 |
041107 |
1003 |
1+ |
041123 |
1507 |
1 |
| 041104 |
2209 |
2+ |
041107 |
1406 |
1+ |
041124 |
0759 |
1+ |
| 041105 |
0555 |
1+ |
041107 |
1513 |
1 |
041124 |
0834 |
2 |
| 041105 |
1016 |
1 |
041107 |
1554 |
2 |
041124 |
1721 |
1- |
| 041105 |
1129 |
1+ |
041107 |
1605 |
1+ |
041124 |
1844 |
1- |
| 041105 |
1635 |
1- |
041107 |
1633 |
3 |
041129 |
0144 |
1 |
| 041105 |
1721 |
2 |
041108 |
0838 |
1- |
041130 |
0655 |
2+ |
| 041105 |
1825 |
1+ |
041108 |
1435 |
1- |
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| 041105 |
1902 |
1- |
041108 |
1547 |
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 |
| J Winkler |
A50 |
NAA NML |
| D Toldo |
A52 |
NAA NWC VTX |
| S Hansen |
A59 |
NAA |
| J Ellerbe |
A63 |
ICV |
| P King |
A80 |
FTA |
| W Moos |
A84 |
FTA |
| M Hill |
A87 |
NAA |
| J Mandaville |
A90 |
NPM |
| G DiFillipo |
A93 |
DHO HWU |
| T Poulos |
A95 |
NAA |
| R Battaiola |
A96 |
HWU |
| J Wallace |
A97 |
NAA |
| M King |
A99 |
HWU |
| P Campbell |
A100 |
NLK |
| G Bressan |
A101 |
HWU |
| F Steyn |
A102 |
NAA NWC |
| L Observatory |
A107 |
DHO |
| P Mortfield |
A108 |
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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November proved to be another active month, especially at the beginning. There was a total of 73 correlated SID events. Many of these had a lower importance rating but still represented a lot of activity for a sun near solar minimum. The GOES-12 spacecraft recorded a total of 225 X-Ray Events. Of these, two were X-Class and 15 were M-Class events, all in the first 10 days of the month. The 5th, 6th and 7th were the most active days.
If you look at the SID Section of the AAVSO website you will notice a new look. I have spent the last month working upgrading the form and content to be more organized and comprehensive. This is to benefit new observers interested in getting into SID monitoring but may also be of help to seasoned observers as I have added a few more sections I would like to add to this over time to include links to any of your personal SID related websites if you have them, and I also would be happy to add articles describing your equipment if it is specialized and you think it would be of interest to others. If you are interested in contributing, please contact me.
I had an interesting experience with noise pickup here at my home the past few months. All of a sudden I started getting very strong noise superimposed on my data charts. It was also very odd looking when looked at closely, exhibiting a very strange periodic behaviour. The noise would be there all day sometimes and some days never. It turned out it was usually on the weekends, and with a little deductive reasoning and some experimenting, I realized it was a new air ionizer that my wife had gotten and was running, usually on the weekends upstairs. Using a program called SpectraLab that runs with my computer sound card I could examine the spectrum and saw that the emissions from the ionizer were at a number of discrete frequencies below 24Khz and one just about at 24Khz, the source of my problem since I monitor NAA at that frequency. On the next page is a set of graphs showing the nasty noise these devices produce as well as a spectrum shot showing the noise spectra.
Noise produced from air ionizer while monitoring NAA at 24 Khz
Here is the spectrum measured using SpectraLab and my computer sound card.The time scale is across the bottom with a vertical frequency range from 0-24Khz. Note the periodic ionizer turn-on which comes in bursts of two and at each burst, one of which is captured by the plot on the right, there is a noise spike at 23.5, 12.1, 11.5, and 6.2 Khz. The two lines near the top are at 21.7 and 20.6 Khz. Clearly Air Ionizers should not be used near a VLF SID Monitoring antenna !!
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