\contentsline {table}{\numberline {1}{\ignorespaces Selected key parameters of the CEBAF 12\nobreakspace {}GeV Upgrade}}{35}
\contentsline {table}{\numberline {2}{\ignorespaces The design characteristics of the MAD spectrometer shown along with HRS performance.}}{37}
\contentsline {table}{\numberline {3}{\ignorespaces CLAS$^{++}$: acceptance and resolution}}{41}
\contentsline {table}{\numberline {4}{\ignorespaces CLAS$^{++}$: operating luminosity }}{41}
\contentsline {table}{\numberline {5}{\ignorespaces HMS performance and SHMS specifications}}{44}
\contentsline {table}{\numberline {6}{\ignorespaces Summary of the GlueX detector's characteristics.}}{46}
\contentsline {table}{\numberline {7}{\ignorespaces Photoproduction cross sections}}{63}
\contentsline {table}{\numberline {8}{\ignorespaces Comparison of the figure of merit for large $x$ measurements of the $A^n_1$ structure function at HERA, SLAC, and JLab.}}{102}
\contentsline {table}{\numberline {9}{\ignorespaces Leading twist transverse momentum dependent distribution functions}}{139}
\contentsline {table}{\numberline {10}{\ignorespaces CLAS$^{++}$ Program Summary - Quark Transverse Momentum and Nucleon Orbital Angular Momentum in Semi-inclusive DIS }}{144}
\contentsline {table}{\numberline {11}{\ignorespaces The values of nuclear transparencies for J/$\psi $ propagation}}{166}
\contentsline {table}{\numberline {12}{\ignorespaces Parameters for the SLAC E158 experiment from the proposal compared to those for a potential Jefferson Lab experiment at 12\nobreakspace {}GeV. }}{193}
\contentsline {table}{\numberline {13}{\ignorespaces Projected uncertainties for ongoing SLAC E158 (from the proposal) and for a potential Jefferson Lab measurement at 12 \nobreakspace {}GeV. }}{194}
\contentsline {table}{\numberline {14}{\ignorespaces Possible sources of systematic uncertainty in the measurement of $A_d$.}}{198}
\contentsline {table}{\numberline {15}{\ignorespaces The design characteristics of the MAD spectrometer shown along with the HRS performance.}}{214}
\contentsline {table}{\numberline {16}{\ignorespaces The parameters necessary to evaluate the cryogenic stability by the Steckly criteria for the MAD Magnets}}{222}
\contentsline {table}{\numberline {17}{\ignorespaces Properties of the large-acceptance spectrometer magnets. }}{223}
\contentsline {table}{\numberline {18}{\ignorespaces Performance estimates for the MAD spectrometer}}{225}
\contentsline {table}{\numberline {19}{\ignorespaces The first-order TRANSPORT matrices in natural units (m) for various configurations of the MAD spectrometer}}{227}
\contentsline {table}{\numberline {20}{\ignorespaces MAD detector parameters}}{230}
\contentsline {table}{\numberline {21}{\ignorespaces Single rates in MAD detector (kHz) with $E_{beam}$ = 11\nobreakspace {}GeV , $I_{beam}$ = 70\nobreakspace {}$\mu $A, and a 15\nobreakspace {}cm long liquid hydrogen target.}}{231}
\contentsline {table}{\numberline {22}{\ignorespaces Geometrical specifications for scintillator planes.}}{233}
\contentsline {table}{\numberline {23}{\ignorespaces Collection efficiency of photons for each phototube.}}{235}
\contentsline {table}{\numberline {24}{\ignorespaces The momentum threshold to produce \v {C}erenkov radiation.}}{237}
\contentsline {table}{\numberline {25}{\ignorespaces Equipment needed for the triggering system of the MAD detector package}}{240}
\contentsline {table}{\numberline {26}{\ignorespaces Comparison of Pb-Glass, PbF$_2$, and PbWO$_4$ calorimeter properties.}}{241}
\contentsline {table}{\numberline {27}{\ignorespaces Key parameters of Beam Quality - present and with upgrade}}{243}
\contentsline {table}{\numberline {28}{\ignorespaces Central Electromagnetic Calorimeter parameters}}{251}
\contentsline {table}{\numberline {29}{\ignorespaces Rise time for various PMTs. The existing CLAS detector uses XP2262 PMTs.}}{268}
\contentsline {table}{\numberline {30}{\ignorespaces Properties of several scintillators. The existing CLAS detector utilizes BC-408 scintillator.}}{268}
\contentsline {table}{\numberline {31}{\ignorespaces HMS Performance and SHMS Specifications}}{281}
\contentsline {table}{\numberline {32}{\ignorespaces Q1 comparison between HMS at 1010 A and SHMS at 1291 A. }}{284}
\contentsline {table}{\numberline {33}{\ignorespaces SHMS QD30 Magnet Parameters. }}{289}
\contentsline {table}{\numberline {34}{\ignorespaces SHMS Optics Parameters for SSA and LSA Tunes}}{299}
\contentsline {table}{\numberline {35}{\ignorespaces Sensitive Areas of the Detectors}}{307}
\contentsline {table}{\numberline {36}{\ignorespaces Nominal Dimensions of the Hodoscope Elements}}{313}
\contentsline {table}{\numberline {37}{\ignorespaces Operating parameters for an experiment using the coherent bremsstrahlung beam.}}{346}
\contentsline {table}{\numberline {38}{\ignorespaces Rates and Processing Requirements}}{347}
\contentsline {table}{\numberline {39}{\ignorespaces Estimation of the experimental uncertainties for $\Gamma (\eta \rightarrow \gamma \gamma )$ measurement.}}{359}