Javascript must be enabled to continue!
Watheroo Magnetic Observatory April to June, 1933
View through CrossRef
April 30‐May 2 1933—This magnetic storm of moderate intensity began at 16h 27m 50s on April 30 with a sudden commencement which was very definitely recorded in all three elements. During the half‐hour preceding the commencement there appeared on all the traces rapid fluctuations of small amplitude; the la Cour rapid trace showed the period of these oscillations to be about 90 seconds and their average amplitude (semi‐range) about 2γ. In the sudden commencement a decrease in H of about 2γ was followed immediately by an increase of 33γ within 5 minutes. In Z the initial impulse represented a slight increase of the force followed by a decrease of 12γ in six minutes. The declination increased westerly at the time of commencement and immediately showed an easterly swing of about one minute of arc in three minutes of time. Irregular movements of only moderate intensity follow in all three elements and continued until 0h 30m on May 1; then followed a quiet period of 12 hours after which what was presumably the same disturbance again became manifest by large irregular movements in all elements, continuing until 2h on May 2 when the traces resumed their normal appearance. It is during this last period of the disturbance that the maximum ranges occurred. The ranges were: Declination 24″; horizontal intensity, 125γ; vertical intensity, 144γ. Time of commencement was taken from the la Cour horizontal‐intensity trace; the Mitchell inductometer showed time of commencement also as 16h 27m 50s. All times are Greenwich mean time.
American Geophysical Union (AGU)
Title: Watheroo Magnetic Observatory April to June, 1933
Description:
April 30‐May 2 1933—This magnetic storm of moderate intensity began at 16h 27m 50s on April 30 with a sudden commencement which was very definitely recorded in all three elements.
During the half‐hour preceding the commencement there appeared on all the traces rapid fluctuations of small amplitude; the la Cour rapid trace showed the period of these oscillations to be about 90 seconds and their average amplitude (semi‐range) about 2γ.
In the sudden commencement a decrease in H of about 2γ was followed immediately by an increase of 33γ within 5 minutes.
In Z the initial impulse represented a slight increase of the force followed by a decrease of 12γ in six minutes.
The declination increased westerly at the time of commencement and immediately showed an easterly swing of about one minute of arc in three minutes of time.
Irregular movements of only moderate intensity follow in all three elements and continued until 0h 30m on May 1; then followed a quiet period of 12 hours after which what was presumably the same disturbance again became manifest by large irregular movements in all elements, continuing until 2h on May 2 when the traces resumed their normal appearance.
It is during this last period of the disturbance that the maximum ranges occurred.
The ranges were: Declination 24″; horizontal intensity, 125γ; vertical intensity, 144γ.
Time of commencement was taken from the la Cour horizontal‐intensity trace; the Mitchell inductometer showed time of commencement also as 16h 27m 50s.
All times are Greenwich mean time.
Related Results
Magnetic cloak made of NdFeB permanent magnetic material
Magnetic cloak made of NdFeB permanent magnetic material
In the past few years, the concept of an electromagnetic invisibility cloak has received much attention. Based on the pioneering theoretical work, invisibility cloaks have been gre...
Astronomical research in Kharkiv at the end of the 19th century – the first half of the 20th century
Astronomical research in Kharkiv at the end of the 19th century – the first half of the 20th century
The main milestones of the formation and development of astronomical science in Kharkiv during 1883–1945 are reconstructed on the example of the activities of the astronomical obse...
Fieldwork teaching on Mars using a Large-Scale Visualisation System
Fieldwork teaching on Mars using a Large-Scale Visualisation System
Recent orbital and rover images of the surface of Mars provide exceptional high-resolution views of the martian landscapes and its surface geology. These extensive datasets provide...
The Earth's magnetic field variations at the Algerian magnetic observatory of Tamanrasset from 1932 to 2020.
The Earth's magnetic field variations at the Algerian magnetic observatory of Tamanrasset from 1932 to 2020.
<p>In order to understand the spatial and temporal behavior of the Earth's magnetic field, scientists, following C.F. Gauss initiative in 1838 have established observ...
The prospects for the implementation of the Pulkovo Observatory observational program at the Assy-Turgen observatory
The prospects for the implementation of the Pulkovo Observatory observational program at the Assy-Turgen observatory
The progress of the observational programs of the Pulkovo observatory involves the transfer of some of them to regions with conducive astroclimatic conditions. The ability of the A...
Watheroo Magnetic Observatory April to June, 1948
Watheroo Magnetic Observatory April to June, 1948
(Latitude 30° 19′.1 S., longitude 115° 52′.6 or 7h 43m.5 E. of Gr.)No magnetic storms of any consequence were recorded at Watheroo during April, May, and June, 1948....
Localized nanoscale induction by single domain magnetic particles
Localized nanoscale induction by single domain magnetic particles
AbstractSingle domain magnetic nanoparticles are increasingly investigated as actuators of biological and chemical processes that respond to externally applied magnetic fields. Alt...
Is the nuclear attraction just magnetic moment interaction between nucleons?
Is the nuclear attraction just magnetic moment interaction between nucleons?
Abstract
By reexamining the magnetic moment interaction between nucleons, it is argued in this article that the formula for calculating magnetic induction generated by magn...

