In searching for the info... Eye injuries of early solar observers -
https://aty.sdsu.edu/vision/others.htmlhttps://en.wikipedia.org/wiki/Thomas_Harriot#Sunspots
> Harriot observed the sunspot with the use of a telescope in a direct and hazardous way. ... Specifics as to how Harriot's telescope was set up remains largely unknown.
This lead me to http://galileo.rice.edu/sci/observations/sunspots.html
> Scheiner, a Jesuit mathematician at the university of Ingolstadt (near Augsburg), wished to preserve the perfection of the Sun and the heavens and therefore argued that sunspots were satellites of the Sun. They appeared as black spots when they passed in front of the Sun but were invisible at other points in their orbits. Their orbits had to be very close to the Sun for their shapes were foreshortened as they approached its edge. Scheiner observed sunspots through a telescope equipped with colored glasses.
> ...
> It was Castelli who developed the method of projecting the Sun's image through the telescope, a technique that made it possible to study the Sun in detail even when it was high in the sky.
This was a very rapid development. https://en.wikipedia.org/wiki/Benedetto_Castelli
> In December 1610, Galileo received a letter from Castelli, asking if the phases of Venus were observable through Galileo's new telescope.
This then lead lead me to https://brunelleschi.imss.fi.it/itineraries/multimedia/Helio...
> In his work on sunspots dated 1613, Galileo refers to the method invented by Benedetto Castelli for observing through the telescope and drawing—without damage to his eyes—the spots that he had discovered on the Sun's surface.
> Galileo darkens the room and aims the telescope at the Sun. At about one meter from the eyepiece, he places a sheet of white paper. The solar disk is thus projected on the sheet. To heighten the contrast of the image and thus make it easier to observe, Galileo places a darkening screen around the sheet. He now draws a circle on the sheet with the compasses and, moving the sheet closer or farther away, he finds the position where the Sun's image exactly overlaps the circle. He then marks the sunspots on the sheet. Since the Sun moves, the helioscope itself must be moved continuously in order to keep the solar image in the circle.