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Post by sigurdur on May 11, 2021 3:43:12 GMT
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Post by douglavers on May 11, 2021 8:50:46 GMT
As a politically incorrect comment, there is a view that people who glue themselves to pavements/roads/railings etc should simply be left there, with suitable precautions to make sure they are not damaged by traffic.
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Post by missouriboy on May 11, 2021 13:02:30 GMT
As a politically incorrect comment, there is a view that people who glue themselves to pavements/roads/railings etc should simply be left there, with suitable precautions to make sure they are not damaged by traffic. Only politically incorrect with "the glued".  Yes ... a look to safety and a little friendly banter. "Good morning brother. You appear to be stuck. My sister did that once. The glue came loose in about a week. Lost some skin too. Kinda cold (warm) out. And it may rain. Did you bring your umbrella? Need anything? I'll be back by 5. Don't run away."  |
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Post by missouriboy on May 11, 2021 13:19:44 GMT
There should now be nearly 30 years of these data, which, for some reason, are not readily available. The abstract comment is consistent with what has been mentioned elsewhere. While TSI (largely the visible spectrum) declines only slightly across cycles, the shorter, more energetic wavelengths show serious variation. These are the exact part of the spectrum which most affect the ozone and penetrate the ocean column to great depths. Such data are seriously damaging to the 0.04 percent solution. Why would these data be so difficult to aquire? Or am I incompetent? These observations indicate almost a factor of two variation near Lyman-α (121.6 nm), decreasing to less than 10% near 200 nm, and to less than 1% near 300 nm. |
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Post by nautonnier on May 11, 2021 20:12:17 GMT
There should now be nearly 30 years of these data, which, for some reason, are not readily available. The abstract comment is consistent with what has been mentioned elsewhere. While TSI (largely the visible spectrum) declines only slightly across cycles, the shorter, more energetic wavelengths show serious variation. These are the exact part of the spectrum which most affect the ozone and penetrate the ocean column to great depths. Such data are seriously damaging to the 0.04 percent solution. Why would these data be so difficult to aquire? Or am I incompetent? These observations indicate almost a factor of two variation near Lyman-α (121.6 nm), decreasing to less than 10% near 200 nm, and to less than 1% near 300 nm.Also note the careful use of 'a factor of two' 50%? then only to percentages when they get small. Classic propaganda approach. |
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Post by sigurdur on May 11, 2021 23:59:28 GMT
There should now be nearly 30 years of these data, which, for some reason, are not readily available. The abstract comment is consistent with what has been mentioned elsewhere. While TSI (largely the visible spectrum) declines only slightly across cycles, the shorter, more energetic wavelengths show serious variation. These are the exact part of the spectrum which most affect the ozone and penetrate the ocean column to great depths. Such data are seriously damaging to the 0.04 percent solution. Why would these data be so difficult to aquire? Or am I incompetent? These observations indicate almost a factor of two variation near Lyman-α (121.6 nm), decreasing to less than 10% near 200 nm, and to less than 1% near 300 nm.Nope, far from incompetent!! I have tried to find data, is how I found the paper. The data is somewhere, not publicly available?? |
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Post by missouriboy on May 12, 2021 2:48:54 GMT
There should now be nearly 30 years of these data, which, for some reason, are not readily available. The abstract comment is consistent with what has been mentioned elsewhere. While TSI (largely the visible spectrum) declines only slightly across cycles, the shorter, more energetic wavelengths show serious variation. These are the exact part of the spectrum which most affect the ozone and penetrate the ocean column to great depths. Such data are seriously damaging to the 0.04 percent solution. Why would these data be so difficult to aquire? Or am I incompetent? These observations indicate almost a factor of two variation near Lyman-α (121.6 nm), decreasing to less than 10% near 200 nm, and to less than 1% near 300 nm.Nope, far from incompetent!! I have tried to find data, is how I found the paper. The data is somewhere, not publicly available?? Ya think they might not trust us to be properly educated (indoctrinated)? It seems like the cloud experiment data. After about 2004, it just disappeared. While I'm sure that clouds are extracted from imagery as a matter of course for other purposes, no one is assembling them in a format useful to "outside" users. |
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Post by sigurdur on May 12, 2021 6:15:25 GMT
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Post by nautonnier on May 12, 2021 14:08:05 GMT
That will take a lot of digging through Sig. |
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Post by missouriboy on May 12, 2021 23:39:29 GMT
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Post by sigurdur on May 13, 2021 2:57:34 GMT
That will take a lot of digging through Sig. Don't have time to investigate. Stumbled across the link. For the next few weeks, you fellers go at it! |
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Post by nonentropic on May 13, 2021 3:17:02 GMT
Not sure but if you go to say 230nm the el nino or something stands out, how?  it's space for god's sake. |
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Post by sigurdur on May 16, 2021 16:06:16 GMT
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Post by duwayne on May 20, 2021 16:43:06 GMT
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Post by missouriboy on May 20, 2021 17:42:11 GMT
Now they can tackle the strength and the length. |
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Yes ... a look to safety and a little friendly banter. "Good morning brother. You appear to be stuck. My sister did that once. The glue came loose in about a week. Lost some skin too. Kinda cold (warm) out. And it may rain. Did you bring your umbrella? Need anything? I'll be back by 5. Don't run away." 
it's space for god's sake. 