Date
1 - 14 of 14
illumination
Robert Moore
The differences between the sensitivity of the human eye and onboard
satellite instruments is quite striking with MSG-1 at the moment. Current visual imagery of Europe obviously shows low levels of illumination - and indeed darkness north of ... whatever the current latitude is. Yet here in N. Wales, even under quite heavy cloud, everything is bright (if not particularly cheerful). Our eyes seem much better at responding to lower levels of light than the instruments. On the other hand, we aren't very good at seeing things by infrared! If I haven't got this all wrong then a question follows: Are there any ways in which we might use our software to squeeze a little bit more out from the visible wavelengths at the darkest parts of the year? I'm not at all clear about this. I appreciate, of course, that one can't enhance something that is not there. David (T) and others, do you have any thoughts on this, or am I wasting everyone's time with the question? Robert ------------------------------ Robert Moore tel and fax: 44 (0) 1352 714456
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maxrpunkt
i don't know if i understood your question correctly, but i think histogram equalization of the visible images could solve your problem.
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johnrigsec@...
In a message dated 20-11-03 16:10:38 GMT Standard Time,
rsmoore@liverpool.ac.uk writes: Yes I was thinking how I can see as easily at summer noon and after dark inRobert, No, MSG will never image by moonlight but at last years EUMETSAT conference there were serious suggestions about doing just that in the next generation of geostationary satellites. Trouble is that imaging via moonlight requires an enormous aperture radiometer - which in turn requires an enormous satellite. Regards, John Tellick. RIG.
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fvalk <fvalk@...>
Robert,
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I agree with you that much of the information that may be used to visualise aspects that are there are lost in the visible light channels. For MSG this is the current situation and for HRPT it has been. We resolved it for HRPT quite some time ago by developing an algorithm that deals with both visible and infrared information. It might be a thought for David to consider incorporating the same principle for MSG as well. David, what do you think? Ferdinand
---------- Original Message -----------
From: Robert Moore <rsmoore@liverpool.ac.uk> To: MSG-1@yahoogroups.com Sent: Thu, 20 Nov 2003 12:32:18 +0000 Subject: [MSG-1] illumination The differences between the sensitivity of the human eye and onboard------- End of Original Message -------
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a_van_belle
Here are my two pennies:
MSG (SEVERI) does send 10 bits grey values (0…1023). Not all these values are used however. Because of the JPG limitations MDM scales these down to 256. Applying a gamma on a low light image does give poor results. But under MDM's advanced setup you can change the min and max value for every channel separate. This way the 256 grey values are better distributed and gamma can be applied, depending on the season. Using XRIT2PIC (which can handle the full 10 bits) I determined the most used Min and Max value for every channel. By setting these in Advanced setup, MDM does utilise the available spectrum much better. Here are my values: Ch01=MAX=891,MIN=43,GAM=140 Ch02=MAX=806,MIN=60,GAM=145 Ch03=MAX=710,MIN=43,GAM=100 Ch04=MAX=756,MIN=53,GAM=100 Ch05=MAX=742,MIN=86,GAM=100 Ch06=MAX=645,MIN=74,GAM=100 Ch07=MAX=829,MIN=74,GAM=100 Ch08=MAX=801,MIN=150,GAM=100 Ch09=MAX=799,MIN=88,GAM=100 Ch10=MAX=800,MIN=102,GAM=100 Ch11=MAX=787,MIN=150,GAM=100 Ch12=MAX=822,MIN=68,GAM=135 By the way, automatic equalisation is nice on HRPT images, but can be annoying on MSG animations ! Greetings, Arne van Belle
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--- In MSG-1@yahoogroups.com, "a_van_belle" <a.van.belle@h...> wrote:
Here are my two pennies:The minimum value for any channel on MSG-1 is currently 51 (0..1023) Because of the JPG limitations MDM scales these down to 256.If there was enough interest, the full ten bits could be delivered in the Professional version of the MSG Data Manager. Most present- day image formats and processing tools can only handle 8-bit images, indeed they eye can only see about 6 bits. Applying a gamma on a low light image does give poor results.value for every channel separate. This way the 256 grey values are better distributed and gamma can be applied, depending on the season. Seasonal adjustments are an excellent idea! The default values of gamma and minimum level are carefully chosen so that black is black, and a single level change above black in the 0..1023 domain will be reflected as a single level change in the 8-bit final image. [] Here are my values:[] Greetings,It's great to hear the results of your experiments, but why do you set the black level on these channels different to what is transmitted (i.e. 51)? A word of warning to anyone making such adjustments in to ensure that your monitor is correctly - see: http://www.jasc.com/monitor1.asp Cheers, David
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Our eyes seem much better at responding to lower levels of lightthan the instruments. Robert, Our eyes (and ears) have a log response, the scientific instruments on MSG-1 demand a linear response. If Log (signal) were transmitted over the link all your prayers would be answered! Ah, assuming the data source has a low noise and a precisely-set black level, that is! Cheers, David
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Robert Moore
Yes I was thinking how I can see as easily at summer noon and after dark in
winter with a full moon. The latter level of illumination is a minute fraction of the former - yet no MSG vis imagery by moonlight! Robert Quoting David Taylor <david-taylor@blueyonder.co.uk>: Our eyes seem much better at responding to lower levels of lightthan the instruments. ------------------------------ Professor Robert Moore Department of Sociology, Social Policy and Social Work Studies The University of Liverpool Eleanor Rathbone Building Bedford Street South Liverpool L69 7ZA tel and fax: 44 (0) 1352 714456
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maxrpunkt
i know that automatic equalization is not reasonable for sequences because of the permanently changing histogramms of the images. that is why i'm doing a 'fixed' histogram equalization. this means i figured out what exactly happens while histogramm equalization of a 12:00 image. this histogram transform is describable by a spline interpolation through a few points (f.e. 20). in this way the resulting image sequences are looking fine. i attached an example of my color composit, where this histogram transform was applied.
max
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Guy Martin <agm@...>
Also the human eye sees in monochrome at low light levels. Rods and cones !!
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Cheers, Guy
----- Original Message -----
From: Robert Moore To: MSG-1@yahoogroups.com Sent: Thursday, November 20, 2003 4:06 PM Subject: Re: [MSG-1] Re: illumination Yes I was thinking how I can see as easily at summer noon and after dark in winter with a full moon. The latter level of illumination is a minute fraction of the former - yet no MSG vis imagery by moonlight! Robert ---------- http://www.gordano.com - Messaging for educators.
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a_van_belle
--- In MSG-1@yahoogroups.com, "David Taylor" <david-taylor@b...>
wrote: The minimum value for any channel on MSG-1 is currently 51 (0..1023)Looking closely at the 10 bit histogram on current HRIT images I cannot detect this lower limit anymore. (it was there on the initial image processing system IIPS) If there was enough interest, the full ten bits could be deliveredimages, indeed they eye can only see about 6 bits.Saving 10 bits would increase the needed storage space too ! It's great to hear the results of your experiments, but why do youI forgot to mention that I tweaked the ch1,2,3 values a bit to get a good balance in the R3G2B1 False Colour images. False Colour is a matter of taste, but I am very pleased with the new settings (better than the values I used before). Below are my Min/Max/Gamma values for FSD (except GOES9=8bit) G10vis=min9,max688,gam135 G10ir=min150,max910,gam100 G10wv=min150,max625,gam100 G12vis=min0,max886,gam135 G12ir=min150,max975,gam100 G12wv=min150,max644,gam100 These values are chosen to maintain all info and spread it as best as possible into the saved 256 greyscales. Note that min150 is the Min value upperlimit, not the value I read on the histogram ! Greetings Arne van Belle
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--- In MSG-1@yahoogroups.com, "a_van_belle" <a.van.belle@h...> wrote:
--- In MSG-1@yahoogroups.com, "David Taylor" <david-taylor@b...>(0..1023) Looking closely at the 10 bit histogram on current HRIT images Iinitial image processing system IIPS)The 51 offset is still there. You will find that the look-at-space parts of the image are no longer set to 51 (but zero as I recall). The 51 is still defined in the prolog. [] Note that min150 is the Min value upperlimit, not the value I readon the histogram ! I'll increase the lower limit maximum, then up to 240 or so, and reduce the upper limit minimum for the next (beta) version. Cheers, David
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a_van_belle
--- In MSG-1@yahoogroups.com, "David Taylor" <david-taylor@b...>
wrote: I'll increase the lower limit maximum, then up to 240 or so, andThanks for that David, I will try this Beta with the ideal values. Will send you the 10 bits histograms I made later. Greetings, Arne van Belle
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OK, that beta is now up on the Web site.I'll increase the lower limit maximum, then up to 240 or so, andThanks for that David, I will try this Beta with the ideal values. Cheers, David
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