As it came to be, I hauled a nice batch of positions on several objects: Lacrosse 5 (05-016A), the Lacrosse 5 r/b (05-016B), the STSS Demo 2 (09-052B) and the NOSS 3-2 (03-054A & C) duo. I also photographed the NOSS 3-4 duo but the image was too much hampered by cliuds tp reliably measure it. I lost amongst others Lacrosse 4 and the STSS Demo 1 to clouds (the latter a pitty, as it was predicted to pass right through the Pleiades).
Most of the images have some clouds on them: some extensively. Below are a few pictures: from top to bottom they show the Lacrosse 5 r/b amidst clouds; The NOSS 3-2 duo passing between the Pleiades and the Hyades; and the STSS Demo 2 passing near capella and the three Goats:
click images to enlarge
![](https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiE3VNQI2bHmQ7YbX_C4TPQI4Ea7fnCkEpEwuMuSQCiPvhBM2W0MijTeLXcVnwCTJoy_AWMjxJmS9i4NKFRFO45oER-GYsJNlReOTOHO3KoFCUM2qwDVb5-nP0z9SHRAB6E5khoow/s280/20022010_Lac5r.jpg)
![](https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEiVvkeCdtqCrS6J8hDwxYfEg54vEDhvKFk47zzUyVCzqSrD_DOYCe5ZAbGV6ItYzh9w4sRxmxYE_JAbyrsTScAm7H_i5cAKtkrPIimsoAklDRpxhzC3TxmdAE0_ho__MNHG0-RSVQ/s280/20022010_NOSS3_2.jpg)
![](https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhy5uzIY_BS5q1-7F97Xl1JA0m6-p7F7F0OqoFUEuee1ZpmuvJHcaj_h4U4HOILare9ep21N2oILxHRmx07rDA48oQNxAtfwYFcL_sEI-SUBngD83oWOcUaRHobPi6LHtuaXpvS7A/s280/20022010_STSS_demo_2_a.jpg)
The STSS Demo 2 appears to show an unusual brightness variation in the first 2 seconds of the trail (the left part of the trail in below negative image), consisting of what appear to be a series of even spaced modest glints. Note the dashed appearance of the first part of the trail:
click image to enlarge
![](https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhaREEGSyZxJg93GWaZ2EsbyG_uYSfadspfyX3LbmZLOP82t4pBJPmazxp77jsFFZQ9rrckcnXJHVP0buKNJKvmsQGOohNPg9RBWAW3APKDgneqa9OVMPPNarWuJ9Ani2WxYuabGQ/s280/20022010_STSS_demo_2_b.jpg)
Below is the brightness profile over the trail (grey small crossmarks are individual pixel values, the solid line is a 3 point average), and below that is a graph of the time between brightness maxima visible in the profile.
click diagrams to enlarge
![](https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEjahxknGaAiU3AxReTSoBKkKRG0JOOATc3-p7hy_BA8CPm3OELBb_2TDYAx_yrzBpWcwITwdKl4C60NGAj1k430PQO0YFb1NipLjLgejxi2oKXgmUWQqoJU7CKSdnKRDaIra8eq_w/s280/STSS_dem2_20feb2010.jpg)
![](https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEhORrSG661auFqQHAGCloTl5qA86et5oZtC4_1W6I2cHkyb5yArVAh8luSrKWAwxlqhxunRPqXa1eIFjtZSTrIo9Yp4-Qi8T20XiFLN_TazFLyreDsllB9CU47hKfMPJji9tNnTIA/s280/STSS_dem2_20feb2010_period.jpg)
Note in the second diagram how the time between maxima is very constant, at about 0.13 seconds, during roughly the first 2 seconds . After that, it begins to wildly vary. As the first diagram shows, the amplitude of the brightness variations is larger in those first 2 seconds too. In fact, after those first two seconds the variation is largely or completely random pixel variation.
The first 2 seconds of the trail are quite different in character from the rest of the trail though: a clear constant, larger amplitude pulsing behaviour. This is very interesting. A second image obtained on the STSS Demo 2 during the same pass showed a quite constant brightness.
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