All the accessible auroral observations recorded in Chinese and Japanese histories during the interval AD 1840–1911 are investigated in detail. Most of these auroral records have never been translated into a Western language before. The East Asian auroral reports provide information on the date and approximate location of each auroral observation, together with limited scientific information on the characteristics of the auroral luminosity such as colour, duration, extent, position in the sky and approximate time of occurrence. The full translations of the original Chinese and Japanese auroral records are presented in an appendix, which contains bibliographic details of the various historical sources. (There are no known rel...
The two great auroral displays of August 28-29 and September 1-2, 1859 are studied from a collectio...
While low-latitude auroral displays are normally considered to be a manifestation of magnetic storms...
The uniquely beautiful light display of an aurora is the result of charged particles colliding with ...
All the accessible auroral observations recorded in Chinese and Japanese histories during the interv...
Early auroral observations recorded in various oriental histories are examined in order to search f...
Comprehensive catalogues of ancient sunspot and auroral observations from East Asia are used to iden...
The validity of a technique developed by the authors to identify historical occurrences of intense g...
A further study is made of the validity of a technique developed by the authors to identify histori...
Aims. Historical records provide evidence of extreme magnetic storms with equatorward auroral extens...
Given that a strong 14C variation in AD 775 has recently been suggested to be due to the largest sol...
SIGLEAvailable from British Library Document Supply Centre- DSC:8715.1804(CCLRC-RAL-TR--95-073) / BL...
“SEKKI ” phenomena often appear in the Japanese historical literatures as distinct red emission in t...
A compilation of records of the aurora observed in China from the Time of the Legends (2000 - 3000 B...
The earliest known drawing of sunspots appears in The Chronicle of John of Worcester, which was comp...
During a great magnetic storm on Feb 11, 1958, a fan-shaped aurora was photographed at Memambetsu, H...
The two great auroral displays of August 28-29 and September 1-2, 1859 are studied from a collectio...
While low-latitude auroral displays are normally considered to be a manifestation of magnetic storms...
The uniquely beautiful light display of an aurora is the result of charged particles colliding with ...
All the accessible auroral observations recorded in Chinese and Japanese histories during the interv...
Early auroral observations recorded in various oriental histories are examined in order to search f...
Comprehensive catalogues of ancient sunspot and auroral observations from East Asia are used to iden...
The validity of a technique developed by the authors to identify historical occurrences of intense g...
A further study is made of the validity of a technique developed by the authors to identify histori...
Aims. Historical records provide evidence of extreme magnetic storms with equatorward auroral extens...
Given that a strong 14C variation in AD 775 has recently been suggested to be due to the largest sol...
SIGLEAvailable from British Library Document Supply Centre- DSC:8715.1804(CCLRC-RAL-TR--95-073) / BL...
“SEKKI ” phenomena often appear in the Japanese historical literatures as distinct red emission in t...
A compilation of records of the aurora observed in China from the Time of the Legends (2000 - 3000 B...
The earliest known drawing of sunspots appears in The Chronicle of John of Worcester, which was comp...
During a great magnetic storm on Feb 11, 1958, a fan-shaped aurora was photographed at Memambetsu, H...
The two great auroral displays of August 28-29 and September 1-2, 1859 are studied from a collectio...
While low-latitude auroral displays are normally considered to be a manifestation of magnetic storms...
The uniquely beautiful light display of an aurora is the result of charged particles colliding with ...