Since receiving his Ph.D. in cosmic ray physics from Ohio State University, Dr. Griffith has brought expertise in space science, spacecraft modeling, and communications systems together to build stronger tools for space missions. His work supports next-generation mission design as optical communications continue to play a growing role in space operations. Dr. Griffith is also an amateur radio operator and avid astrophotographer, passions which inform his contributions to space observation technologies.
In the 2010s and 2020s, on-orbit optical communications have moved from the realm of technology demonstrations and into practical implementation. And it’s easy to see why, since its very short wavelengths offer the following advantages over traditional radio frequency (RF) communications:
• Reduced size, weight, and power
• Comparable or better data rates compared to RF
• Better physical security, owing to a narrow beam spot at ground level which is more difficult to intercept

screenshot from https://youtu.be/Ma5PSu5wg_E – 0:14
So for the correct application, moving to optical communications from RF can truly allow you to achieve more with less.
But what are some challenges associated with optical comms?
When answering this question, it’s useful to consider a mathematical expression called the “link margin,” which consists of “gains” (which make the connection easier to close), and “losses” (which make it harder to close). The link margin can be thought of as a sum, where each term is a gain (positive) or a loss (negative), followed by a subtraction of the receiver sensitivity. If the link margin is positive, your link is achievable at the performance level you’ve indicated, but if it’s negative, you’ll have to find some way to make up the difference.
In an optical link the gains are provided by the:
• Transmitter (think of the narrow beam of a laser pointer, it’s this intense focus that makes a lot of the “magic” of optical comms possible)
• Receiver (this is basically a telescope, and the diameter of it sets the gain)
For losses we have free space loss, which is unavoidable and the same as in RF comms, but we also have a number of atmospheric effects that we must now take into account. These consist of:
• Atmospheric absorption (not modeled in FreeFlyer, but can be disregarded if we choose a wavelength which falls within one of the transparent “windows” of Earth’s atmosphere; 1550 nm is a very popular choice)
• Atmospheric scattering (modeled in FreeFlyer by a straightforward parameterization using widely available meteorological visibility measurements)
• Atmospheric scintillation (modeled in FreeFlyer via a turbulence path integral; this a signal “wobble” caused by pockets of warm air in the atmosphere, it’s also what makes my planet pictures blurry!)
Oh, and before I forget! Another important source of loss is the mechanical precision of the component which points your laser transmitter. As you might imagine, the narrower you make your laser beam, the more precise your pointing must be, so I’ve made sure to model this important tradeoff in FreeFlyer as well.
As you can see there are quite a large number of parameters that go into considering the performance of an optical comms system, so FreeFlyer gives you the ability to either flexibly represent your current system, or sketch out a new one which meets your needs, all the way from site selection, to topics we haven’t even talked about yet like modulation choice.
It’s been a real a thrill to work on this feature, and I can’t wait to see what you do with it! To help you get acquainted with all the new elements related to optical communication simulation, FreeFlyer 7.10 comes with a number of sample mission plans that show off various capabilities. These include:
1.) A model of a walker constellation employing optical links between satellites

2.) A scenario exploring the effect of different modulation choices on an optical link between a lunar lander and a ground station on Earth

Screenshot from https://youtu.be/peoydVFk-t4 - 01:20
3.) An example of how the presence of a bright celestial object (e.g. Venus) in the field of view of can degrade optical receiver sensitivity


