For a full understanding of the dynamics of the Ionosphere it is preferable to consider the whole gamut of contributors. Contributors such as Ionospheric composition and dynamics requires determination of factors beyond TEC such as atomic and molecular species concentration, Ion-based contributions and how they interact and correlate with the radiation belts, and even solar events. Atomic and molecular species concentration requires a study of specific abundance measurements in each layer as a function of altitude and geographical distribution. Similarly, ion-based contributions require a study of concentrations associated with relevant species as a function of altitude and geographical distribution. We study the available concentration of these contributors to further understand their interactions within the Ionosphere. The desired outcome of this study is to drive the field to generate a new set of requirements to attain better space situational awareness and understanding.