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Archives

Two black-and-white images of the planet, with the axis or rotation aligned left to right. Belts, including a darker equatorial region, are well seen.

Uranus during the 2016 apparition

A report by the Uranus Coordinator of the BAA Saturn, Uranus & Neptune Section (Director: Mike Foulkes) This report describes

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In the centre-band image, filaments and bright plage is more clearly seen; the flare appears bright against the dark umbrae and penumbrae of the active region

Observations of a major solar flare, revisited

Hydrogen-alpha observations of a major flare from 2003 November are revisited.   Introduction 2023 November marks the 20th anniversary of

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The brighter comets of 2020

A report of the Comet Section (Director: N. D. James) This report describes and analyses the observations of the brighter

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From the BAA Archives

Towards the end of 2022, the BAA Trustees agreed to fund the development of an Archives website. Its main purpose

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A chronology of some lunar drawings by Galileo Galilei

By taking into consideration the morphological features along the terminator in some of Galileo’s watercolour portraits of the Moon, found

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Noctilucent cloud over Thurso in Scotland, with silhouetted house in foreground

Noctilucent cloud over Britain & Western Europe, 2022

Noctilucent cloud forms in the mesosphere at an altitude of about 83km and appears annually in northern latitudes between the

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A colour image of the variable reflection nebula NGC 6729, taken by Terry Evans. It appears blue-ish, with some black absorption nebulosity occluding also visible and occluding the background stars

Brightness variations in R CrA & NGC 6729 during 2021

An indicative luminance light curve for R CrA created from data collected during 2021 showed a brightness range between magnitudes

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Rippling clouds of electric blue set against a dark northern sky, tinged with light as if twilight.

Auroral & noctilucent cloud activity, 2023 June 19 – August 18

With coronal mass ejections and sunspot numbers regularly in triple figures, the odd X-class flare and several coronal holes, the

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The y axis gives the signal to noise ratio (SNR) and the x axis gives the epoch numbers. Each SNR curve starts low and tends towards a flat higher number as the epoch number increases

Image denoising in astrophotography – an approach using recent network denoising models

Image denoising is an important consideration for improving the accuracy of acquired data. Given the morphological nature of astrophotography, with

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A star field containing the dwarf nova in outburst

The 2021 superoutburst of the dwarf nova LL Andromedae

We present photometry of the 2021 outburst of LL And, which was only the fourth confirmed on record, with a

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