Magnetic field and plasma observations from magnetotail passes of the AMPTE
/IRM satellite are used to study the low-frequency magnetic fluctuation ene
rgy density as a function of several local plasma parameters. Two statistic
al constraints on this quantity are found, one a function of proton pressur
e, one a function of proton flow speed, suggesting that ion-driven electrom
agnetic instabilities may contribute to the observed fluctuations.