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Starts

Here you can select the time from which the observations will be displayed. The last month will be used by default. In this case, the search results in the middle of the page will show the findings reported to the Skywarden during the past month.

By clicking on the word 'ends' with the mouse, you will also see the end time of the search period. This is useful in situations where you want to look at observations from a period in the past, such as reports from a particular week in Skywarden.

Especially when looking at observations for a particular time period, you may want to do the search based on when the observed phenomenon actually happened instead of the time when it was sent to the observation database. In that case, you may want to select 'Observed' instead of the default 'Sent'. Please note that the browser uses a cookie to remember your choice of the start time of the search. If you have enabled cookies and do not clear them from your browser's cache, the same browser will display observations from the same time window you last selected the next time you use it.

Please note that the browser uses a cookie to remember your choice of the start time of the search. If you have enabled cookies and do not clear them from your browser's cache, the same browser will display observations from the same time window you last selected the next time you use it.

at

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The "Sent" -option retrieves observations submitted to the Skywarden during the selected time period, regardless of when those phenomena were seen in the sky.

The selection “observed” retrieves the phenomena that appeared in the sky during the selected period, regardless of when they were reported to the Skywarden.

2000-01-02 00:00 == 2022-07-02 07:53

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You can choose to show only phenomena of the desired level of visibility in the search results. For example, "at least III" removes the phenomena classified as the weakest (I-II). Similarly, "at least V" removes from the results all but the relatively rare phenomena or those classified as very impressive (V).
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Here you can do a free-text search to the observations

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You can search for any persons observations by writing the observer's whole name or part of the name here. For example 'John Smith' or 'John S'

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To find observations made in some specific location, type the municipality name to the search field. For example, "Mikkeli"

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In this field, you can search for more detailed phenomenon identifiers included in the observation details.

Such are, for example, deep space object types such as "spiral galaxy" or "reflection nebula" or halo forms such as "sundog" or "sun pillar".

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Newest observations

Turku, Lightning photo IV
2.7.2022 at 04.00
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1.7.2022 at 22.16
Riihimäki, One halo form I
1.7.2022 at 16.45
Kangasala, One halo form I
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Kangasala, Several halo forms II
1.7.2022 at 14.02
Turku, Primary rainbow III
1.7.2022 at 06.04
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1.7.2022 at 01.20
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1.7.2022 at 01.00
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30.6.2022 at 22.50 1
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Contact information

Skywarden,
Ursa Astronomical Association

Kopernikuksentie 1
00130 Helsinki

taivaanvahti(at)ursa.fi

Sun - 6.7.2014 at 16.30 Luoto Observation number 27211

Visibility III / V

Pekka Ruohomäki, Katternö skywatchers

There are a lot of spots in the sun and a new unnamed spot still looms in the northeast on Sunday night.

This description has been automatically translated from Finnish. Click here to see the original text.

Auringossa paljon pilkkuja ja itäkoillisessa häämöttää uusi vielä sunnuntai iltana nimeämätön pilkku.

6 6

Additional information

Observation target
- Sun
- Keskitaso

Technical information

Ha image: Lunt LS60THa B1200CPT, DMK 51AU02 Polka dot image: Skywatcher Mercury-705 + Astro Solar visual film + Baader's green cdd filter. DMK 51AU02

Twiittaa

Report this

Comments: 2 pcs

Rauno Päivinen - 8.7.2014 at 06.01 Report this

Hienoa jälkeä, luntin kuva on erityisen komeaa katseltavaa.

Pekka Ruohomäki - 8.7.2014 at 09.51 Report this

Kiitos. Olen ollut tyytyväinen Luntin suorituskykyyn. Samoin DMK51:een. Olen viimeaikoina kuvannut pinnan gamma arvolla 60 ja proturberanssit gamma arvolla 200 ... 250 suunnilleen samoilla valotusajoilla. Tämä menettely helpottaa kuvankäsitteyä merkittävästi.

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