Philippe Rousselle's SHG
Posted: Sun May 31, 2015 1:51 pm
Hi,
My name is Bob, I live in West Yorkshire, UK and I’m new to the Solar Chat forum. I have a particular interest in the science and observation of our nearest star, our Sun, hence the reason I wished to join Solar Chat.
I’ve taken an interest in understanding the construction and use of the spectrohelioscope and I’ve found fascinating the wealth of information available on this forum. I’m particularly interested in Philippe Rousselle’s SHG adapted from a 115/900 mm Newtonian and after reading the details on his website on astrosurf.com some questions have come to mind which I would hope those who are more knowledgeable than me could answer.
At the moment I’m trying to understand Philippe’s use of the divergent meniscus lens to increase focal length of the telescope. I appreciate the reason for this is to increase the F/D ratio so that the telescope has a greater focal ratio than the collimator. From my understanding a divergent lens produces a virtual image on the same side of the lens as the object image, so the virtual image does not form a visible projection. In this case how can the image of the Sun be seen on the slit to ensure that the image is in focus?
I’ve got other questions, but rather than have lengthy posts I’ll take it a step at a time.
Many thanks, Bob
My name is Bob, I live in West Yorkshire, UK and I’m new to the Solar Chat forum. I have a particular interest in the science and observation of our nearest star, our Sun, hence the reason I wished to join Solar Chat.
I’ve taken an interest in understanding the construction and use of the spectrohelioscope and I’ve found fascinating the wealth of information available on this forum. I’m particularly interested in Philippe Rousselle’s SHG adapted from a 115/900 mm Newtonian and after reading the details on his website on astrosurf.com some questions have come to mind which I would hope those who are more knowledgeable than me could answer.
At the moment I’m trying to understand Philippe’s use of the divergent meniscus lens to increase focal length of the telescope. I appreciate the reason for this is to increase the F/D ratio so that the telescope has a greater focal ratio than the collimator. From my understanding a divergent lens produces a virtual image on the same side of the lens as the object image, so the virtual image does not form a visible projection. In this case how can the image of the Sun be seen on the slit to ensure that the image is in focus?
I’ve got other questions, but rather than have lengthy posts I’ll take it a step at a time.
Many thanks, Bob