Unfortunately in 1859 the Kew Observatory had the only self-recording magnetographs . the manually recorded magnetic readings from the Colaba Observatory for 1 September, through 2 September 1859 were recalibrated and evaluated.
12.
Stewart reported that the magnetic storm from the Stewart Super Flare, began at 22 : 30 GMT on the evening of 28 August 1859 as recorded by self-recording magnetographs at the Kew Observatory.
13.
A vector magnetograph works in a very narrow waveband around a single spectral line, for example the 525.02 HMI instrument on board the Solar Dynamics Observatory will produce a vector magnetogram every few minutes.
14.
Also in the 1950s, Babcock and his father, Harold, who was at Mount Wilson as well, created the first solar magnetograph for measuring the intensity, direction and distribution of the Sun's magnetic field.
15.
The huts included a magnetograph hut, used to measure variations in the south magnetic pole; an absolute magnetic hut, which was used as a reference point for studies in the magnetograph hut; and the transit hut, an astronomical observatory.
16.
The huts included a magnetograph hut, used to measure variations in the south magnetic pole; an absolute magnetic hut, which was used as a reference point for studies in the magnetograph hut; and the transit hut, an astronomical observatory.
17.
The largest geomagnetic perturbation, resulting presumably from a " prehistoric " CME, coincided with the first-observed solar flare, in 1859 . The flare was observed visually by Richard Christopher Carrington and the geomagnetic storm was observed with the recording magnetograph at Kew Gardens.
18.
Stewart did not publish the magnetograph records for the morning of 28 August 1859 . While it is extremely unlikely, the original magnetograph records for that date should be inspected to determine if any disturbance was recorded because of the uncertainties in timings and the nearness of sunrise.
19.
Stewart did not publish the magnetograph records for the morning of 28 August 1859 . While it is extremely unlikely, the original magnetograph records for that date should be inspected to determine if any disturbance was recorded because of the uncertainties in timings and the nearness of sunrise.
20.
Vector magnetographs measure the longitudinal ( line-of-sight ) component of the magnetic field separately from the transverse ( image-plane ) components, using different aspects of the Zeeman splitting that affects the wavelength of emission and / or absorption spectral lines in the presence of a magnetic field.
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