UNITED STATES DEPARTMENT OF THE INTERIOR JUNE 1988 GEOLOGICAL SURVEY PRELIMINARY GEOMAGNETIC DATA COLLEGE OBSERVATORY FAIRBANKS, ALASKA OPEN FILE REPORT 88-0300F BARROW
UNITED STATES DEPARTMENT OF THE INTERIOR
JUNE 1988
GEOLOGICAL SURVEY
PRELIMINARY GEOMAGNETIC DATACOLLEGE OBSERVATORY
FAIRBANKS, ALASKA
OPEN FILE REPORT 88-0300F
BARROW
THIS REPORT WAS PREPARED UNDER THE DIRECTION OF JOHN B, TOWNSHEND, CHIEF OF THE COLLEGE OBSERVATORY, WITH THE ASSISTANCE OF THE OBSERVATORY STAFF MEMBERS: R,V, 0 CONNELL AND L,Y, TORRENCE AND IN COOPERATION WITH THE GEOPHYSICAL INSTITUTE OF THE UNIVERSITY OF ALASKA, THE COLLEGE OBSERVATORY IS A PART OF THE BRANCH OF GLOBAL SEISMOLOGY AND GEOMAGNETISM OF THE U,S, GEOLOGICAL SURVEY,
Explanation of Data and Reports
Magnetic Activity Report
Principal Magnetic Storms
Preliminary Calibration Data and Monthly Mean Absolute Values
Magnetogram Hourly Scalings - Five Quietest Days
Sample Format for Normal and Storm Magnetograms
Normal Magnetograms
Storm Magnetograms (When Normal is too disturbed to read)
COLLEGE OBSERVATORY PRELIMINARY GEOMAGNETIC DATA
EXPLANATION OF DATA AND REPORTS
INTRODUCTION
The preliminary geomagnetic data included here is made available to scientific personnel and organizations as part of a cooperative effort and on a data exchange bards because of the early need by some users. To avoid delay, all of the data is copied from original forms processed at the observatory; therefore, it should be regarded as preliminary. Inquiries about this report or about the College Observatory should be addressed to:
Chief, College ObservatoryU.S. Geological Survey800 Yukon DriveFairbanks, Alaska 99775-5160
Requests for copies of the magnetograms except for the current month should be addressed to:
World Data Center A NOAA D63m 325 Broadway Boulder, Colorado 80303
OBSERVATORY LOCATION
The College Observatory, operated by the U.S. Geological Survey, is located at the University of Alaska, Fairbanks, Alaska. It is near the Auroral Zone and the northern limit of the world's greatest earthquake belt, the Circum-Pacific Seismic Belt. Although the observatory's basic operation is in geo magnetism and seismology, it cooperates with other scientists and organizations in areas where the facil ity and personnel can be of service.
The observatory is one of three operated by the USGS in Alaska. The others are located at Barrow and Sitka.
The position of the observatory site is: Geographic latitute........64° 51.6'NGeographic longitude.......147° 50.2'WGeomagnetic latitude.......+64.6°Geomagnetic longitude......+256.5°Elevation..................200 meters
GEOMAGNETIC DATA
Normal and storm magnetograms and appropriate calibration data are processed at the observatory and are available for analysis or copying. Also available are mean hourly scalings for the five quietest days for the month and K-Indices.
Magnetic Activity
The K-Index; The K-Index is a logarithmic measure ment of the range of the most disturbed component (D or H) of the geomagnetic field for eight intervals 0000-0300, 0300-0600...2100-2400 UT. It is a measure of the difference between the highest and lowest deviation from a smooth curve to be expected for a component on a magnetically quiet day, within a three hour interval.
The Equivalent Daily Amplitude, AK: The K-Index is converted into an equivalent range, ak, which is near the center of the limiting gamma ranges for a given K. The average of the eight values is called equivalent daily amplitude AK. The unit 10y has been chosen so as not to give the illusion of a accuracy not justified.
The schedule for converting gamma range to K, and "K to ak is as follows:
Gamma Range K - Index
25< 50<
10CX 200< 350< 600< 1000
1000< 1650 1650< 2500 2500+
50100200350600
ak~tf
3 7
15274880
140 240 400 (lOy)
Principal Magnetic StormsGradual and sudden commencement magnetic distur
bances with at least one K-Index of 5 or greater, which are believed to be part of a world-wide disturbance, are classified as principal magnetic storms. The time of the storm beginning and ending; direction and amplitude of sudden commencements; period of maximum activity; and storm range are reported. Monthly reports of these data are forwarded to the World Data Center A in Boulder, Colorado.
Magnetogram Hourly ScalingsMagnetogram hourly scalings are averaged for
successive periods of one hour for the D, H, and Z elements. The Value in the column headed "01" is the average for the hour beginning 0000 and ending 0100. Note that the values on the scaling sheet are in tenths of mm with the decimal point omitted. The user of these scalings should keep in mind that the tabular values are hourly means and if one is interested in the detailed morphology of the magnetic field, refer directly to the magnetograms.
MagnetogramsThe normal magnetograms in this report are repro
duced at about one-third the size of the originals. Preliminary base-line values and scale values adopted for use with the original magnetograms are included. For days when the magnetic field is too disturbed for the Normal magnetogram .to be readable, Storm magnetograms are reproduced.
Absolutes, Base-lines and Scale ValuesTo determine the absolute value of the magnetic
field from the hourly means or from point scalings the following equations should be used:
D=BD+d-SD; H=BH+h-SH ; Z=BZ+Z-SZwhere D, H and Z are absolute values;Bp, Br, and B^ are base-linp values;Sp, Su and Sg are scale values;and d, h and z are scalings in millimeters.
*u»AFORM74 133 U. S. DEPARTMENT OF COMMERCE (9-72) /°- | *» NATIONAL OCEANIC AND ATMOSPHERIC ADMINISTRATION
MAGNETIC ACTIVITY(Greenwich civil time, counted from midnight to midnight)
DATE
1
2
3
4
5
6
7
89
10
11
12
13
14
15
16
1718
19
20
21
2223
24
25
26
27
28
2930
K-INDICES
m u? £ CM o o o -i A i &0000
11131202000000001100
44100232232400103432
23321111321045442221
2322
34443222 33365354
11142344232235213454
22343312133615535442
in co - «».- CM CM
A J> A.- CM
10211011000001103232
01111111211133220211
23101000100153330122
311142125432 45323211
41125211211255324 5 3 3
33441 2 3. 132225444666 3
SUM
1008000212
1211161116
1605083112
152423 2924
152215
2631
2516223136
OBSERVATORY
College AlaskaMONTH AND YEAR
June 1988
AK
0503000106
0805090610
0902042805
081817 2821
1017072428
1808193046
TIME SCALE ONMAGNETOGRAMS
20 nun/hr
SUDDEN COMMENCEMENTS
d h m
POSSIBLE SOLAR-FLARE EFFECTS BASED ON
INSPECTION OF GRAMS ALONE (WITHOUT
REFERENCE TO DATAFROM OTHER SOURCES)
BEGIN END
d h m d h m
K SCALE USED: D
LOWER LIMIT FOR K s 9. ........ AT rj
CURRENT SCALE VALUE.......
vx / X 1
3.70LOWER LIMIT FOR K = 9 ........ 2500
SCALINGS AND COMPUTATIONS HAVE BEEN CHECKED.
APPROVED
H Z
322.2 fmm ^
7.79 (7/mm)
2510 (to nearest 107)
John B. Townshend, Chief, College ObservatoryOBSERVER IN CHARGE
NOAA FORM 76-133 SUPERSEDES CftGS FORM 815 U.S. GOVERNMENT PRINTING OFF IC E: 1873-761-857
NQAA
FORM
86-5
00
(11/
73)
Data f
rom
Indi
vidu
al Observatories
IPRINCIPAL MA
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June
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COLLEGE OBSERVATORY, COLLEGE, ALASKA PRELTKIKAHY CALIBRATION I>ATA FGR: June 1988'
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